The galaxy presents as an elongated structure with a noticeable color gradient. A relatively smooth, concentrated core region transitions into a less defined, extended halo. There is evidence of a disk-like structure within this halo, although the resolution limits precise characterization. The galaxy exhibits a bluer hue on one side, suggesting the presence of younger stellar populations. Conversely, the opposite side displays a more reddish tone, likely indicating older stellar populations. There is evidence of disturbed morphology, possibly indicating a past interaction. There is some evidence of a minor tidal disturbance or merger event, potentially contributing to the observed asymmetries and color variations within the galaxy. The galaxy's overall shape deviates slightly from being perfectly round.
