The galaxy presents as a relatively compact, bright object with a noticeable central concentration. The overall morphology appears smooth, with little evidence of strong spiral arm structure or significant dust lanes. There is some evidence of a minor disturbance or perhaps a weak tidal feature on one side of the galaxy, suggesting a possible interaction or recent merger event. The galaxy exhibits a color gradient, with the central region appearing bluer than the outer regions. This color difference could be indicative of ongoing star formation in the core relative to an older stellar population in the outskirts. The overall shape appears fairly round, suggesting that it is likely an elliptical galaxy.
