The galaxy presents a generally smooth, elliptical morphology with a somewhat diffuse appearance. The light distribution is concentrated towards the center, displaying a bright, unresolved core region. There is little indication of spiral arm structure or prominent dust lanes. The overall color is slightly redder in the outer regions, transitioning to a bluer hue closer to the galactic center. The galaxy appears largely undisturbed, without significant tidal features or signs of a major merger event. A slight asymmetry in the outer isophotes may suggest a minor interaction or internal dynamic process. The galaxy exhibits an apparent angular size corresponding to a physical diameter on the order of several kiloparsecs. Star formation appears to be present, though not dominant, suggesting a mixed stellar population with a significant contribution from older stars.
