This galaxy presents as a relatively smooth, elliptical or lenticular structure. Its shape is elongated, exhibiting a cigar-like morphology rather than a perfect circle, with a high degree of central concentration. The central bulge appears prominent, displaying a bright core that fades gradually into the outer regions of the galaxy.

The color profile indicates a possible mixture of stellar populations. The inner region shows a slightly reddish tint, suggestive of older, cooler stars. The outer areas are slightly bluer, possibly indicating more recent star formation, albeit at a low rate, or the presence of younger, hotter stars.

There is no visual evidence of spiral arms or a well-defined disk, which aligns with its smooth appearance. The absence of significant dust lanes or irregular features suggests that this galaxy is relatively undisturbed. There are no signs of recent major mergers or strong tidal interactions.

The galaxy’s overall appearance points toward a system where the majority of stars formed early in its history, and current star formation is minimal. The high degree of smoothness and central concentration may indicate that this is a relatively evolved galaxy, possibly transitioning towards a quiescent state.
