The galaxy presents as a generally smooth, elliptical-like structure with a slightly elongated morphology. The central region exhibits a concentrated luminosity, suggesting a prominent bulge. The galaxy appears to transition smoothly from the core to the outer regions, though there is subtle hint of a possible disk.

There appears to be some blue tinges in the surrounding disk, suggesting the presence of younger, hotter stars. It may be possible that these regions have active star formation, though star formation is quite limited overall. There appears to be no disturbances in morphology.
