The galaxy presents as a primarily smooth, elliptical morphology. Its shape appears to be somewhere between round and elongated. The galaxy exhibits a color gradient from a yellowish core to a greenish outer region, which may indicate differing stellar populations or dust content. There are no obvious signs of spiral arms or a distinct disk structure. The overall appearance suggests a relatively evolved system, with limited ongoing star formation. There are no obvious signs of a major merger, though there is a slight asymmetry to the galaxy, possibly indicating a recent minor interaction. The estimated size of the galaxy is a few kiloparsecs in radius.
