The galaxy appears as a moderately bright, relatively smooth object. It exhibits an elliptical morphology with a notable lack of spiral arm structure. There is an indication of a slight color gradient, with a somewhat yellower hue concentrated toward the core region of the galaxy, possibly indicating an older stellar population. This transitions gradually to a bluer, less intense halo, which could suggest the presence of a younger stellar population or ongoing star formation at a low rate. The overall structure appears somewhat disturbed, showing possible signs of tidal interactions or a minor merger event that may be influencing the morphology. The galaxy's light profile is somewhat diffuse, with no prominent central point source.
