The galaxy presents as a relatively compact, elliptical-like structure. Its morphology appears predominantly smooth, with no immediately discernible spiral arms or prominent dust lanes. The light distribution suggests a centrally concentrated spheroid, with a gradual decrease in luminosity towards the outer edges. The galaxy exhibits a yellowish-red color profile, potentially indicative of an older stellar population and a relatively low rate of ongoing star formation. The galaxy appears relatively isolated. Overall, the galaxy appears as an evolved system.
