The galaxy presents as a luminous object with a complex morphology, exhibiting characteristics of both a smooth spheroid and a disk-like structure. A bright, concentrated central region is evident, possibly indicating the presence of a galactic bulge. Surrounding this central core, a fainter, more diffuse region extends outward, showing hints of spiral arm structure, although these features appear somewhat disturbed or irregular. The color gradient suggests potential variations in stellar populations or dust content across the galaxy, with a possible shift towards bluer hues in the outer regions, possibly denoting ongoing star formation. The overall structure suggests a galaxy undergoing or having recently undergone an interaction or disturbance, contributing to its somewhat amorphous shape and complex internal dynamics.
