The galaxy presents as a centrally concentrated, elliptical-like structure. Its core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The outer regions appear fainter and slightly more diffuse, with subtle extensions that indicate some tidal disturbance. There is a noticeable absence of well-defined spiral arms or prominent dust lanes, which supports an early-type classification. Overall, the galaxy appears relatively smooth, although there is a hint of asymmetry potentially due to minor gravitational interaction. There is some indication of ongoing, albeit low, star formation.
