The galaxy presents as a single, somewhat elongated structure, appearing more cigar-shaped than round. A bright central region dominates the galaxy's overall luminosity. The central region shows a yellow or orange hue, suggesting an older stellar population and a reduced rate of star formation. Extending outward from the central area, there are indications of fainter, bluer regions, particularly on the outskirts of one side. This suggests some ongoing star formation, though it is not widespread. The galaxy seems to be undergoing a significant disturbance, possibly a merger event, given its irregular shape and the presence of these extended features. There appear to be signs of some tidal tails, but more information would be necessary to confirm.
