The galaxy presents a generally smooth and rounded morphology, exhibiting a concentrated central bulge. The color profile appears to be predominantly redder, suggesting an older stellar population. There are no apparent spiral arms or a disk-like structure. The overall structure indicates a system that may be approaching a more elliptical form. Visual inspection suggests the possibility of tidal features or a slight disturbance, which warrants further investigation into its merger history. Further analysis is required to determine if this object is currently undergoing, or has undergone, a merger.