The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears bright white, suggesting a high density of older stars. The overall morphology is largely undisturbed, with no obvious signs of ongoing major mergers.

There's a distinct blue tint emanating from the central region, indicative of some level of active star formation. This could be due to the presence of younger, hotter stars. A slight hint of a disk-like structure can be inferred, although it isn't prominently featured. The shape is notably round. Possible minor disturbances are visible, with a small amount of irregular light distribution.
