The galaxy presents as a centrally concentrated, relatively smooth object with a subtle color gradient. It appears elliptical or lenticular in shape, displaying a slightly elongated profile. The core region exhibits a bright, yellowish-white hue, indicative of an older stellar population. Moving outwards from the core, the color shifts towards a slightly redder tone. The outer regions appear fainter and more diffuse, with a trace of disk-like structure. There appears to be very little resolved structure present, such as spiral arms or prominent dust lanes. Overall, this galaxy seems to be a fairly evolved system with a dominant bulge component. There is little evidence of ongoing major star formation. There may be minor tidal disturbances.
