The galaxy presents a largely smooth, elliptical morphology, exhibiting a centrally concentrated luminosity profile. The core region appears bright and yellowish-white, indicating a population dominated by older stars. There is a slight elongation, but the overall shape is relatively round. Subtle color gradients can be observed, transitioning from a slightly bluer hue in the outer regions, indicative of pockets of more recent star formation, to a redder center, suggesting an older stellar population and reduced star formation. The absence of well-defined spiral arms or a prominent disk suggests a more evolved system. Faint, extended light surrounds the main body of the galaxy, hinting at a diffuse halo of stars. There is no apparent evidence of ongoing major mergers or significant tidal disturbances, although some minor irregularities in the outer halo cannot be ruled out based on this image alone.
