The galaxy presents as a centrally concentrated object, with a generally smooth appearance indicative of an elliptical or lenticular morphology. The light distribution is concentrated in the core, showing a bright central region, with a relatively high degree of circularity. There is a slight elongation along one axis, though the overall shape is nearly circular.

Color gradients within the galaxy appear subtle. The central region exhibits a slight blue hue and the outer regions appear somewhat redder. This suggests the presence of ongoing, though perhaps not exceptionally vigorous, star formation activity within the central region, with older, redder stellar populations dominating the outskirts. Overall, the galaxy appears to be a relatively quiescent system with a modest amount of star formation. There is no obvious evidence of major interactions or mergers that would significantly disturb its overall structure.
