The galaxy presents as an elliptical morphology, appearing generally smooth with minimal discernible substructure. The light distribution suggests a concentrated central bulge that diffuses outwards. Color gradients indicate a possible aging stellar population, with a yellowish hue dominating the core, potentially indicative of older, redder stars. The outer regions exhibit a bluer tint, implying the possibility of ongoing, albeit subdued, star formation. There is no readily apparent spiral arm structure or distinct dust lanes present, and no signs of active galactic nucleus activity. The galaxy exhibits a regular shape, showing no major signs of gravitational disturbance or recent major merger events, with only faint, slight irregularities.
