The galaxy appears to be a relatively smooth, elliptical-like system. The morphology suggests minimal disk-like features or spiral arms. It exhibits a centrally concentrated luminosity profile with a smooth gradient outward from the core. The central region is brighter and more yellow in color, indicating a concentration of older stellar populations. The outer regions become progressively fainter and appear slightly bluer, which could be due to some level of ongoing star formation, although limited. Overall, the galaxy presents a rather undisturbed morphology, with no clear signs of major mergers or significant tidal disturbances. It appears relatively isolated, showing no obvious signs of interaction with other galaxies. The galaxy has a moderate size.
