The galaxy presents as a luminous central region with a somewhat diffuse, extended halo. The core exhibits a yellowish-white hue, suggesting an older stellar population. Evidence of possible tidal features or disturbances can be seen. These could indicate gravitational interactions with neighboring galaxies, or remnants of a past merger. A portion of the galaxy appears flattened and elongated, though without defined spiral arm structures, suggestive of a lenticular or early-type spiral classification. The galaxy's overall morphology appears primarily smooth, but has notable irregularities. The object appears relatively massive, and shows moderate star formation activity.
