The galaxy presents as a primarily smooth, elliptical-like structure. It exhibits a concentrated central bulge that is bright and gradually fades into a more diffuse halo. There is a slight asymmetry to the galaxy's overall shape, with a subtle extension or tidal feature visible on one side. This could be the sign of a minor disturbance or a past merger. The color distribution suggests an older stellar population, with a higher concentration of redder stars in the central regions. No distinct spiral arms or significant dust lanes are observed. The galaxy appears relatively isolated, without any obvious close companions that may be gravitationally interacting with it.
