The galaxy appears as a somewhat diffuse object with an apparent flattened or disk-like structure, seen at an oblique angle relative to our line of sight. The central region exhibits a slightly brighter, concentrated luminosity, potentially indicative of a galactic bulge or nucleus.

The overall color profile suggests a mixed stellar population, with some regions showing bluer tints which could correspond to areas with ongoing or recent star formation. The smoothness of the light distribution is moderate, with some subtle irregularities and possible hints of spiral arm structure, but there does not appear to be defined spiral arms. There is some indication of minor disturbances or tidal features in the galaxy's morphology, which could suggest interactions with smaller objects.
