The galaxy presents a predominantly smooth morphology, with a concentrated central bulge. The overall color appears bluish, particularly in the central region, suggesting the presence of a relatively young stellar population. There is a hint of a flattened disk-like structure surrounding the bulge, but the disk lacks distinct spiral arms or detailed features. A slight asymmetry is observed, potentially indicating a minor interaction or disturbance. The outer regions appear fainter, transitioning to a redder hue. The overall light distribution suggests that it is not undergoing major merger activity. 
