The galaxy presents as a well-defined, elongated structure with a smooth, centrally concentrated light distribution. The morphology suggests a likely classification as an elliptical galaxy, although a highly inclined spiral cannot be ruled out without further data. The overall color appears relatively uniform, hinting at an older stellar population. There is a slight color gradient visible, with a bluer central region and a redder halo. There is no evidence of strong star formation regions, major disturbances, or prominent dust lanes. The galaxy appears to be relatively isolated, showing no obvious signs of interaction with neighboring galaxies. The galaxy's estimated size is approximately 4 kiloparsecs across its half-light radius.
