The galaxy appears to be a roughly elliptical or lenticular system, with a concentrated central bulge. There is no discernible spiral arm structure. The light profile suggests a relatively smooth distribution, although some faint, asymmetric extensions are present, possibly indicative of minor tidal disturbances or interactions. The color is generally consistent across the galaxy, with a slight reddening towards the central region. Overall, this galaxy shows characteristics of an evolved system, likely with an older stellar population.
