The galaxy presents a largely smooth, elliptical morphology with minimal discernible disk structure. It appears as a concentrated spheroid of light, with a bright central core region that gradually fades towards its outer edges. The color profile indicates an older stellar population, with a yellowish-red hue dominating the central bulge region. There is a slight bluer tint to the outer edges, suggesting a younger population of stars, but it could also simply be an artifact. There is very little evidence of active star formation regions or prominent spiral arm structures, although there seems to be a very slight asymmetry. The overall impression is one of an evolved system, with very little signs of ongoing major mergers or interactions, though there may be a slight disturbance in the outer halo.
