The galaxy appears to be a smooth, elliptical-like structure, likely an early-type galaxy based on its uniform color and lack of prominent spiral arms or dust lanes. It exhibits a slight elongation, appearing somewhat cigar-shaped rather than perfectly spherical. The light distribution is concentrated toward the center, with a bright, diffuse core that fades gradually outward. The color is predominantly yellow-orange, suggestive of an older stellar population with minimal ongoing star formation. There is no visible evidence of recent mergers or major disturbances in its structure, although a very slight asymmetry might indicate a minor interaction in the past.
