The galaxy presents as a fairly smooth, rounded object with a concentrated central region that is noticeably brighter and exhibits a yellowish hue. The overall color suggests a population of older stars dominating its stellar content. A fainter, more diffuse halo surrounds this central region, displaying a slightly bluer tint, possibly indicating the presence of younger stellar populations or ongoing star formation at the edges. There is a subtle hint of a disk-like structure, though not distinctly defined. No significant morphological disturbances, such as tidal tails or merging features, are readily apparent, suggesting a relatively quiescent evolutionary state.
