The galaxy presents as a relatively bright, somewhat elongated, disk-like structure. There is a central bulge region that appears yellowish, likely indicating an older stellar population. The disk component is bluer in hue, suggesting ongoing star formation. The galaxy lacks any apparent tightly wound spiral arms. There is a slight lopsidedness to the overall shape, and there is potential for minor distortions. The galaxy is not undergoing a major merger and does not appear to be an elliptical galaxy.
