The galaxy presents as a relatively compact, ellipsoidal object. Its overall color is a mix of green, red, and blue, suggesting moderate star formation activity with the presence of both older stellar populations and younger, bluer stars. A diffuse halo appears to surround the central region, though it is not particularly extensive. There is no obvious spiral arm structure visible, although the slight elongation suggests a disk-like morphology. Some potential disturbances are visible in the main body of the galaxy suggesting a possible minor merger event. Overall, the galaxy exhibits a somewhat disturbed morphology that may be due to internal or external factors.
