The galaxy exhibits a relatively smooth morphology, appearing largely spheroidal in shape with a moderate concentration of light towards the center. The color gradient suggests an aging stellar population, with a yellowish hue dominating the central regions. A fainter, bluer extension appears adjacent to the galaxy, possibly indicating a region of more recent star formation or a tidal feature resulting from a minor interaction. There is no distinct spiral arm structure visible; the galaxy is likely an elliptical or lenticular type. The overall structure appears largely undisturbed, with no obvious signs of a major ongoing merger, although subtle asymmetries might indicate a past interaction. The galaxy is estimated to be of intermediate mass. The rate of star formation is low.
