The galaxy presents as a centrally concentrated object with a smooth morphology. Its shape is roughly elliptical, exhibiting a slight deviation from perfect circularity. The color profile suggests a dominant population of older stars, indicated by the yellowish hue. There is no visible evidence of spiral arms, dust lanes, or prominent star-forming regions. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers with other galaxies in its immediate vicinity. It is a relatively luminous galaxy.
