The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish hue, suggesting an older stellar population. The outer regions fade into a faint halo, displaying a redder color, possibly indicating a mix of older stars and dust. There is no readily apparent spiral arm structure or significant dust lane obscuration. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers or tidal disturbances, though a very slight asymmetry in the outer halo cannot be ruled out as a minor interaction. It has a seemingly regular shape; it is round in appearance.