The galaxy presents as a generally smooth, elliptical form. The light distribution appears concentrated towards the center, exhibiting a brighter, yellowish core, likely indicating a higher density of older stars. The outer regions gradually fade into a diffuse halo. While a slight elongation can be observed, the galaxy lacks distinct spiral arm structures or prominent features indicating active star formation. There is some indication of minor disturbance of its shape, though this could be due to its interaction with a potential companion galaxy not clearly resolved in this image. The galaxy appears to be relatively isolated in its immediate environment.
