The galaxy presents as a luminous, relatively smooth, and centrally concentrated object. It appears largely elliptical in shape, displaying a high degree of radial symmetry. The light distribution indicates a dominant bulge component with a smooth transition into the outer regions. Faint, diffuse extensions or tidal features are not readily apparent, suggesting no recent major merger events. The color is generally consistent, showing a somewhat yellowish to reddish hue indicative of an older stellar population. There's no clear evidence of distinct spiral arm structures or regions of active star formation within the observable light. The overall morphology is consistent with a quiescent, early-type galaxy.
