The galaxy exhibits a relatively small angular size. It possesses a disk-like structure, though the disk appears somewhat disturbed or irregular. A central, bright bulge is observed, which is indicative of a concentration of older stars. The color distribution suggests varying stellar populations within the galaxy. The central bulge is redder in color, potentially from older stars, while regions within the disk exhibit bluer hues, suggesting ongoing star formation. There is evidence of possible minor disturbances present, such as tidal features or asymmetries in the disk's structure. There is no clear spiral arm structure is seen. 
