The galaxy presents as a centrally concentrated object, exhibiting a smooth, spheroidal morphology. There is a dominant bulge component which gradually fades outwards, with an apparent lack of distinct spiral arm structures or prominent dust lanes within the optical image.

The galaxy displays a color gradient, with a slightly redder hue towards its core, suggesting an older stellar population in the central region. The outer regions exhibit a bluer color, possibly indicating the presence of younger stars or ongoing star formation activity.

Based on the smooth light distribution and overall morphology, the galaxy appears to be an elliptical galaxy, or possibly an early-type spiral galaxy with a dominant bulge. There is no visual evidence of any major mergers or tidal disturbances in the immediate vicinity of the galaxy. The outer regions appear relatively undisturbed and smoothly distributed.
