The galaxy presents as a lenticular or early-type spiral galaxy, viewed at a moderate inclination. It exhibits a smooth, centrally concentrated bulge that dominates the galaxy's overall luminosity profile. A flattened disk component is visible, though it lacks distinct spiral arm structures. The central region is yellowish to orange, possibly indicating an older stellar population. Moving outward, the disk appears bluer, which may be related to sporadic star formation. The galaxy appears relatively isolated, without clear signs of tidal interactions or major mergers, though there may be a minor disturbance. Overall, the galaxy appears to be in a relatively quiescent state, showing characteristics that are between spiral and elliptical galaxies, or a late stage spiral galaxy.
