The galaxy presents as a largely smooth, elliptical-like structure. There is a strong central concentration of light, exhibiting a yellowish-orange hue, possibly indicative of an older stellar population. The light fades gradually towards the galaxy's outer regions, suggesting a lack of prominent spiral arms or distinct features. While mostly homogenous, there is a slight hint of bluer tones in the outermost regions. The galaxy is generally round in appearance, with no obvious signs of significant tidal distortion or ongoing major mergers. However, there may be some subtle disturbances or minor interactions visible in the faint outer regions. Overall, the galaxy appears to be a fairly evolved system with a dominant bulge component and a relatively quiescent star formation history.
