The observed galaxy presents a disk-like morphology, viewed at a slight angle, which appears to be close to face-on but still shows some depth. A prominent central bulge region is evident with a diffuse stellar distribution that gradually fades outward towards the edges of the galaxy. Within the disk, indications of spiral arm structure are present, though somewhat ill-defined. The arms appear flocculent and lack the clear, grand-design structure often seen in spiral galaxies. The spiral arms display a bluer hue. The galaxy appears to have undergone some disturbances in the past, or is in the process of some interaction. There may be some merging activity. The overall color index indicates ongoing star formation, and the central bulge seems to have some degree of intermediate age stars. There is no evidence of a strong bar structure within the disk.
