The galaxy exhibits an elliptical morphology, appearing as a somewhat elongated spheroid of light. The core region displays high luminosity, with a smooth, centrally concentrated light profile. Moving outwards from the core, the luminosity gradually decreases. The overall color profile suggests a population of older stars, contributing to the yellowish hue observed. There is a faint indication of a disk-like structure or possibly some faint spiral arms. The galaxy appears relatively undisturbed, with no major signs of recent mergers or tidal interactions. Overall, it presents as a mature galaxy with evidence of a bulge-dominated structure.
