The galaxy appears as a centrally concentrated, elliptical or lenticular structure. Its overall form is smooth with no apparent spiral arm features. The light distribution is relatively uniform. There is a gradual decrease in brightness from the core outward. The galaxy's color appears somewhat redder, potentially indicating a population of older stars, diminished star formation, and/or significant dust content. The morphology suggests a relatively quiescent object with an estimated size of several kiloparsecs across. There is a very slight asymmetry to the light distribution that may indicate a minor gravitational interaction, but appears to be an isolated, settled object.
