The galaxy presents an overall disturbed morphology, suggesting it is currently undergoing, or has recently undergone, a significant merger event. There appears to be a central, somewhat amorphous, bulge exhibiting a yellowish hue. This central region transitions into a broader, more diffuse disk-like component. The disk is not well-defined, lacking clear spiral arm structures. Instead, it shows irregular patches of bluer light indicative of ongoing star formation.

There is a clear asymmetry in the galaxy's structure, with one side appearing more extended and less defined than the other. This could be due to tidal interactions or the remnants of a disrupted companion galaxy. The overall color of the galaxy is relatively uniform, with a slight shift towards redder colors in the central bulge and bluer colors in the outer regions. The galaxy exhibits a moderate size on the sky, with no pronounced tidal tails or other extended features immediately apparent. The disturbed and asymmetrical nature suggests a dynamically active system, likely in the process of evolving through gravitational interactions.
