The galaxy presents as a relatively smooth, centrally concentrated elliptical morphology. The light profile transitions from a bright, yellowish core to a diffuse, fainter halo extending outwards. The galaxy appears elongated, exhibiting a cigar-like shape with a major axis approximately 2-3 times the length of its minor axis. There is little indication of spiral arm structure or significant dust lanes. The overall color suggests a population of older stars, with potentially low levels of ongoing star formation. No signs of major mergers or significant tidal disturbances are evident. The galaxy's structure and color profile point toward a system dominated by an evolved stellar population within a smooth, spheroid-like distribution.
