The galaxy presents as a somewhat distorted spiral or lenticular system. The central bulge exhibits a yellowish-white hue, suggesting an older stellar population dominating the core. A faint disk appears to be present, extending outwards from the bulge. There is a distinct, asymmetric feature on one side of the central bulge that may be evidence of a tidal interaction or merger event, potentially with a smaller satellite galaxy. There are signs of disturbed morphologies, likely ongoing or recent interactions. Low levels of star formation are likely taking place within the galaxy based on its color.
