The galaxy presents as a roughly elliptical morphology, displaying a smooth, centrally concentrated luminosity profile. The core region is a bright, yellowish-white, indicating a population of older stars. Moving outward from the core, the light gradually fades into a bluer, less intense halo. This suggests a possible transition in stellar populations and/or a lower density of stars in the outer regions. While the overall structure appears relatively undisturbed, there are faint hints of asymmetry or minor disturbances in the outer halo, possibly indicating past interactions. There may be ongoing, albeit low-level, star formation activity within the galaxy, predominantly in the less concentrated regions. The size is relatively moderate, indicating a mass range common for galaxies of its type. The redness of the core is greater than the bluer surrounding region, which indicates different stages of stellar evolution between these two regions.
