The galaxy appears as a centrally concentrated object with a smooth, relatively featureless morphology. Its light profile suggests an elliptical or S0 classification. The shape is nearly circular. There is no obvious presence of spiral arms, a bar, or prominent dust lanes. There are no other nearby objects that suggest recent merger events. The galaxy exhibits a subtle color gradient, appearing slightly bluer toward the central region, indicative of ongoing, albeit modest, star formation activity in the core. The overall color suggests a stellar population dominated by older stars.
