The galaxy presents as a somewhat smooth, disk-like structure with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting a population of older stars. There may be some faint spiral arm structures present within the disk but they are difficult to discern. The overall color of the disk appears bluer, indicative of ongoing star formation. There is a possibility that this galaxy is undergoing a minor merger event, indicated by some irregular features. This may be causing some of the increased star formation. The galaxy appears to be relatively massive, suggesting it is a mature system. 
