The galaxy appears as a somewhat diffuse object with a central, brighter region exhibiting a yellowish hue. Extending from this central area are fainter, less structured regions with a slightly bluer tint, potentially indicative of ongoing star formation. The overall morphology suggests a galaxy with a combination of smooth and disk-like features, although the resolution limits detailed analysis of spiral arms or distinct features. There is a suggestion of some minor disturbances within the galaxy's structure, but the galaxy does not appear to be undergoing a major merging event. The object's estimated size is approximately 9 kpc in radius, making it a moderately sized galaxy.
