The galaxy presents as a relatively bright, elliptical structure. The central region exhibits a concentrated, yellowish-white luminosity, suggesting a high density of older stars and a possible supermassive black hole actively emitting radiation. Moving outward from the core, the galaxy transitions into a fainter, bluish-white halo. This halo exhibits a smoother texture, possibly indicative of a lack of active star formation within this region. The galaxy appears largely undisturbed, showing no strong signs of recent major mergers or tidal interactions. There may be slight disturbances, but they are minimal. The overall morphology leans toward an early-type galaxy with a substantial spheroidal component.
