The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge. The outer regions appear less luminous, fading gradually into the background sky. The color profile suggests a population of older stars, as indicated by the yellowish hue in the central region. The galaxy is elongated, but not highly so; it appears more "in between" in terms of roundness. There is no obvious evidence of spiral arms or significant dust lanes. The overall structure appears undisturbed, with no strong indications of recent or ongoing major merger activity. There might be a very minor disturbance or asymmetry in the outer regions, but it is not pronounced.
