The galaxy presents an overall elliptical morphology, though there are signs of disk-like features present. The central region exhibits a concentration of light, appearing yellowish-white, suggesting a population of older stars. Extending outwards from this central bulge, there is a disk which has some disturbances and distortions. The disk appears slightly inclined relative to our line of sight. Faint, blueish regions are visible in the disk, perhaps indicative of ongoing star formation. The galaxy does not appear to be undergoing a major merger, but there are minor disturbances and distortions.
