This galaxy presents an overall elliptical morphology, with a bright, concentrated nucleus suggesting a significant bulge component. The light distribution appears relatively smooth and diffuse, fading gradually from the central region outwards. The galaxy is more intermediate in apparent roundness and ellipticity, being neither perfectly spherical nor highly elongated. There are some indications of potential disturbances, such as subtle asymmetries and faint tidal features, but this is not definitive. Overall, the galaxy is not undergoing a major merger, and it appears largely undisturbed, maintaining its overall structure. The galaxy's color profile is consistent with a population of older stars, with a yellowish-red hue in the central region.
