The galaxy appears to be a spiral type, although the features are somewhat disturbed. The central bulge is bright and concentrated, exhibiting a generally smooth, diffuse light distribution. There appears to be some asymmetry in the overall structure, which could indicate a recent or ongoing interaction with another galaxy. One arm appears more disturbed than the other. There is evidence of some disk-like structure surrounding the bulge. Overall, the galaxy presents a disturbed morphology suggesting possible tidal disruption or a recent merger. The color gradient indicates an active star-forming region with a mixture of stellar populations.
