The galaxy presents as a slightly elongated, lenticular structure with a bright, concentrated central bulge. A relatively smooth distribution of light is observed, with a subtle transition from the core to the outer regions. The overall color appears to be consistent with an older stellar population, exhibiting a yellow/red hue in the central region which transitions to a bluer hue on the outer edges. There is minimal evidence of spiral arms or significant dust lanes. The galaxy seems relatively undisturbed, lacking any obvious signs of ongoing major mergers or tidal interactions, although some mild asymmetry in the outer regions cannot be ruled out entirely. The galaxy exhibits characteristics more closely resembling an early-type galaxy.