The galaxy presents as an elliptical morphology, characterized by a centrally concentrated bulge that fades into a diffuse halo. The color gradient suggests an older stellar population, with the central bulge exhibiting a more pronounced yellow-red hue relative to the surrounding regions. A faint, possible tidal feature or dwarf galaxy companion appears in the lower-left region of the galaxy. This suggests a potential ongoing or past interaction or minor merger. Overall, the galaxy displays characteristics indicative of a relatively quiescent object, with low star formation activity, consistent with an elliptical classification.
