The galaxy presents as a generally smooth and elliptical structure. The core exhibits a concentrated luminosity, appearing yellowish-orange, which may indicate an older stellar population dominating the central region. Moving outwards from the core, the galaxy becomes slightly bluer and less luminous, suggesting the presence of younger stars. The overall shape leans toward being "in between" round and elliptical. There's no visually apparent major disturbances to its structure, and it appears relatively isolated, with no signs of ongoing or recent major merger activity. Faint hints of a possible disk-like structure are very subtly present but this is not a disk galaxy and it appears fairly smooth overall. The color gradients within the galaxy suggest varying ages of stellar populations, with older stars concentrated towards the center and potentially younger populations in the outer regions.
