The galaxy presents as a somewhat diffuse, centrally concentrated object. Its overall morphology appears primarily elliptical, though not perfectly spherical, exhibiting a slightly elongated shape. A smooth, relatively uniform distribution of light is observed across the main body of the galaxy, with a gradual decrease in luminosity from the central core outwards. There are no prominent spiral arms or distinct disk features readily apparent. The color gradient is subtle, with a possibly reddish hue concentrated in the central regions, indicative of an older stellar population. The outer regions appear bluer, which may imply younger stars. Hints of minor disturbances or tidal features are suggested in the outer halo, indicative of past interaction or merger. The galaxy appears relatively isolated, with no obvious companion galaxies in close proximity.
