The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular type.  Its overall color is yellowish-orange, indicating a stellar population that is primarily older, with a relatively low rate of ongoing star formation. The galaxy exhibits a concentrated central bulge, with a gradual decrease in brightness moving outward. There is no discernible spiral arm structure or prominent dust lanes. The shape of the galaxy appears to be somewhat elongated, leaning towards the 'in between' roundness categorization. No signs of major mergers are apparent; however, a slight asymmetry in the outer regions could indicate a minor disturbance or past interaction.
