The galaxy presents with an overall elliptical morphology, showing a smooth distribution of light. It exhibits a bright central bulge, which appears to dominate the structure. Surrounding the bulge is a fainter, more diffuse halo. There is evidence of a disk component. There are slight signs of disturbances, suggesting possible minor interactions, but the primary structure appears relatively unperturbed. No prominent spiral arms or bar features are discernible. The overall color appears somewhat redder, suggesting an older stellar population.
