The galaxy presents an ellipsoidal morphology, with a relatively smooth light distribution. The galaxy appears to have a round shape, which is evident from its observed axial ratios. The galaxy exhibits a generally featureless structure, dominated by a smooth spheroidal component. The galaxy exhibits clear signs of an ongoing merger or tidal interaction. There is a notable absence of prominent spiral arms or well-defined dust lanes, indicating that this is either an elliptical galaxy or a spiral galaxy that is currently merging. There is no clear spiral structure, suggesting that the galaxy is either an elliptical galaxy with a smooth, symmetrical light profile, or a disk galaxy obscured by dust. The color gradient suggests older stellar populations, possibly indicating suppressed recent star formation activity.
