The galaxy appears as a primarily smooth, elliptical structure. There is a concentration of light towards the center, suggesting a prominent galactic nucleus or bulge. The light profile appears to fade gradually outward from the center, without any sharp edges or distinct spiral arms. There appears to be a very small presence of disk-like structure, but it is quite minimal, and the galaxy is dominated by the ellipsoidal component. The overall shape is moderately elliptical rather than perfectly circular. No major signs of recent mergers or significant tidal disturbances are discernible. The galaxy exhibits a color gradient, with the core appearing more yellowish, hinting at an older stellar population, while the outer regions show subtle hints of bluer colors, possibly indicating some ongoing star formation. 
