This galaxy presents a generally smooth morphology, appearing as a somewhat elongated, elliptical structure. The central bulge is prominent, exhibiting a bright, concentrated luminosity with a yellowish-orange hue. The luminosity gradually decreases from the core outward, suggesting a diminishing stellar density within the galaxy's halo. There's a subtle disk-like component, but the overall shape leans more towards a spheroid. Some degree of asymmetry is suggested by a slight elongation along one axis. The galaxy appears relatively undisturbed, showing no strong evidence of ongoing major mergers or tidal interactions. The color profile indicates a population of older stars, with a low rate of star formation activity.
