The galaxy presents as an elliptical morphology, characterized by a centrally concentrated, bright core. The light distribution appears largely smooth with a gradual decrease in intensity from the core outwards. There is a slight elongation in its overall shape, deviating marginally from a perfect circle. No prominent spiral arms or distinct structural features are visible. The color profile suggests a predominantly older stellar population within the central region, indicated by its yellowish-red hue. Fainter, bluer regions are perhaps present in the outer areas, suggesting some recent, though limited, star formation activity. There is no evidence of any major ongoing merger events, although faint asymmetries may suggest minor interactions in its past.
