The galaxy appears to be a relatively small, faint object. Its morphology is somewhat ambiguous, but there are some subtle features present. The primary structure presents a disk-like morphology. Possible indications of minor disturbances can be detected. While the galaxy appears as mostly smooth, close inspection reveals some slight asymmetries or irregularities in its shape and brightness distribution. This might suggest the galaxy is undergoing, or has recently undergone, a minor interaction or merger event. The galaxy's color profile indicates that it is likely composed of both young and old stellar populations.
