The galaxy presents as a somewhat elliptical, yellow-tinged spheroid. Its central region exhibits a bright, concentrated luminosity suggestive of a substantial stellar population and possibly an active galactic nucleus, although the resolution is insufficient to confirm the presence of the latter. The galaxy lacks any distinct spiral arm structures, with its light smoothly decreasing radially outwards from the core. There is a slight elongation of the galaxy, deviating from a perfect circle. The overall color suggests an older stellar population with lower levels of recent star formation. Dimmer, diffuse light surrounds the central core, potentially indicating a halo of older stars and globular clusters. There appears to be some kind of disturbance or interaction occurring with a dimmer, smaller galaxy; this could be the merging of the two galaxies.
