The galaxy presents as a somewhat elliptical, centrally concentrated object. There is a smooth light profile with a lack of distinct spiral arms or other significant features indicating a disk. The core appears bright and yellowish, suggesting a population of older stars and/or dust obscuration. The outer regions of the galaxy exhibit a fainter, more diffuse glow, with a slight bluer tint than the core, potentially indicative of some ongoing star formation. No signs of major mergers or tidal disturbances are immediately apparent, although there may be minor asymmetry. The galaxy's shape is not perfectly round, but appears elongated.
