The galaxy presents as a slightly elongated, elliptical structure with a smooth, concentrated central bulge. The overall color is yellowish-orange, indicative of an older stellar population. There are no prominent spiral arms or dust lanes visible. The galaxy appears relatively undisturbed, lacking signs of recent major mergers, though perhaps exhibiting minor disturbances, and it does not seem to be actively forming many new stars. The morphology is more rounded than cigar-shaped. The galaxy has an estimated size of a few kiloparsecs across. The light distribution suggests a relatively high Sersic index, indicating a centrally concentrated profile.
