The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. There is a notable lack of distinct spiral arms or significant dust lanes within the visible spectrum. The overall color profile exhibits a yellowish-white hue in the central regions, suggesting an older stellar population. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers. There is a very slight asymmetry in the outer halo, though it is very subtle. The galaxy exhibits a high degree of roundness.
