The galaxy exhibits a pronounced elongated, cigar-like morphology. It appears relatively smooth and featureless, with a bright central bulge that gradually fades into the outer regions. The color profile suggests a population dominated by older stars, indicated by the reddish hue, potentially representing a later-type galaxy. There's no apparent spiral structure or distinct dust lanes visible. There are no visible signs of active galactic nuclei. The overall morphology suggests a galaxy undergoing limited recent star formation.
