The galaxy presents as an elliptical or lenticular type, characterized by a predominantly smooth and featureless morphology. It exhibits a centrally concentrated luminosity profile, gradually decreasing outwards. The galactic core appears bright and slightly elongated, with an intermediate degree of roundness transitioning to a more elongated shape further from the center. There is no readily apparent spiral arm structure or significant dust lane obscuration. The overall color index suggests a population of older stars, contributing to the yellowish-orange hue. There is no obvious presence of active galactic nuclei features or signs of major mergers or tidal disturbances in the visible structure. The observed light distribution indicates a system that is relatively stable and relaxed, likely having undergone significant dynamical evolution in the past.
