The galaxy presents as a largely elliptical structure with a smooth, concentrated light profile. The core exhibits a yellowish hue, suggesting a population of older stars. The overall form is quite round. There is a faint, diffuse halo surrounding the central region that fades into the background sky. No distinct spiral arms, dust lanes, or signs of active star formation are readily apparent from the image. There is no obvious disruption to its shape, indicating that this is not a galaxy undergoing a major merger. Slight asymmetry may exist within the outermost reaches of the halo.
