The galaxy presents an elliptical morphology, appearing largely smooth and rounded in shape, exhibiting a high degree of central concentration. There is a noticeable color gradient, with the core region appearing more reddish-orange, suggestive of an older stellar population. Progressing outward, the galactic halo appears yellower. The visible structure is primarily a smooth, spheroidal distribution of light, with no readily discernible spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no strong evidence of ongoing major mergers or tidal interactions. The overall appearance suggests a galaxy dominated by evolved stars, possibly indicative of ongoing, but mild star formation.
