The galaxy presents as a lenticular or early-type spiral galaxy, characterized by a smooth, centrally concentrated bulge. It appears elongated, with a cigar-like shape. A faint disk-like structure is hinted at. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population. Some minor disturbances are visible in the disk, potentially due to minor gravitational interactions. Overall, the galaxy gives the impression of being a relatively massive system with little ongoing star formation.
