The galaxy presents as a lenticular, cigar-shaped object with a smooth, centrally concentrated bulge. It appears relatively undisturbed, exhibiting no clear signs of ongoing major mergers or tidal interactions. The central bulge displays a yellowish-orange hue, indicative of an older stellar population. A faint, flattened disk surrounds the bulge. The disk shows a slightly bluer color, potentially from the presence of some star formation activity, but the dominant population appears to be older stars within the disk as well. There are no obvious spiral arm structures within the disk. Overall, the galaxy appears to be a relatively quiescent, massive system.
