The galaxy presents as a lenticular or early-type spiral galaxy, viewed at a moderate angle. The light profile appears relatively smooth, with a prominent bulge region that exhibits a slightly bluer hue compared to the more yellowish color of the extended disk. There are hints of faint spiral structure within the disk, but the arms are not well-defined. There is evidence of some disturbance, though it does not appear to be undergoing a major merger. The light suggests some amount of recent or ongoing star formation, particularly concentrated within the central bulge.
