The galaxy exhibits a generally smooth morphology, with a slight deviation from perfect circularity. The primary body of the galaxy presents a concentrated central bulge, characterized by a yellow-orange hue, potentially indicating an older stellar population and a lower rate of current star formation. Fainter, bluer regions extend from the main body, potentially signifying areas of more recent star formation. There is no apparent major disruption or merging activity. There is a subtle blueness on the right side of the galaxy.