The galaxy presents as a relatively smooth and elliptical-like structure, displaying a high degree of central concentration. The core exhibits a bright, unresolved nucleus, surrounded by a diffuse halo of light that diminishes in intensity with increasing radius. The color appears yellowish-white across the galaxy, suggesting a population of older stars. There is no apparent evidence of spiral arms, dust lanes, or active star formation regions. The overall morphology indicates that this is likely an early-type galaxy, possibly an elliptical or lenticular galaxy, with a largely quiescent stellar population. There do not appear to be any signs of ongoing major mergers or significant tidal disturbances.
