The galaxy presents as a moderately bright, elongated, and reddish-yellow object. The morphology appears primarily smooth with a possible slight disk-like structure. The color suggests an older stellar population with ongoing but relatively low star formation, consistent with a spiral galaxy that is in its final stages of star formation. The light distribution is concentrated towards the center, which has a cigar-like shape, indicative of a bulge. There are indications of minor disturbances, but no clear signs of a major ongoing merger.
