The galaxy presents as a system with a dominant central component and evidence of ongoing interaction. The core appears relatively smooth and centrally concentrated. The overall form factor tends towards intermediate, neither perfectly spherical nor highly elongated. There's asymmetry present suggesting possible tidal interaction or morphological disturbance. A tidal tail or plume emanating from the main body is suspected to be a second interacting galaxy. The color gradient shows a bluer hue at the core and a redder tint towards the tidal features. The apparent luminosity suggests a galaxy of substantial intrinsic brightness. The overall structure indicates a system experiencing active star formation, likely triggered by an interaction with a nearby galaxy. 
