The galaxy presents as a generally smooth, elliptical structure. There is a concentrated, bright central bulge, exhibiting a yellowish-orange hue, which could be indicative of an older stellar population dominating the core. Surrounding the core is a more diffuse halo, exhibiting a bluer tint. There are no prominent spiral arms or distinct features readily apparent. The overall shape appears somewhat elliptical, with only a slight deviation from circularity. There is no evidence of any major disturbances to the galaxy's morphology, such as tidal tails or obvious signs of ongoing mergers.
