The galaxy presents as a singular, relatively compact object with a largely spheroidal morphology. The luminosity profile appears smooth, with a concentrated bright core that gradually diminishes towards the outer edges. There is very little evidence of spiral arm structures or prominent dust lanes. A faint, diffuse halo surrounds the main body of the galaxy, contributing to its rounded appearance. Subtle color variations are present, with the central region showing a slightly bluer hue compared to the redder outer regions, suggesting possible differences in stellar populations. Overall, the galaxy's features suggest a system with minimal ongoing star formation and a relatively evolved stellar population.
