The galaxy presents as a smooth, elliptical-like structure. It exhibits a concentrated central bulge with a yellowish hue, indicating an older stellar population. Fainter, diffuse regions extend outwards, suggesting a less dense distribution of stars in the outer regions. The overall shape is somewhat elongated, hinting at a possible mild distortion. There is a subtle colour gradient from the core outwards, with the outer regions appearing slightly bluer, potentially indicative of younger stars. There are no apparent spiral arms or significant dust lanes visible. The galaxy appears relatively isolated, with no obvious signs of major interactions with other galaxies.
