The galaxy presents as a relatively compact, centrally concentrated object. It exhibits a generally smooth morphology, lacking prominent spiral arms or a pronounced bar structure. The overall color appears reddish, indicating a population dominated by older stars and a lower rate of star formation. There is some subtle irregularity to the galaxy's shape, which, combined with what appears to be a tidal tail and possible disruption of light from the core of the object, indicates a strong likelyhood of ongoing or recent merger.

Based on its size and characteristics, the galaxy appears to be of an intermediate mass range.
