The galaxy presents an overall smooth morphology, appearing largely featureless. It exhibits a concentrated central bulge which transitions into a more diffuse, extended halo. The shape appears generally elliptical but is somewhat difficult to determine precisely given the image resolution. There's a subtle color gradient, with the central region appearing slightly bluer than the outer halo, which could indicate a difference in stellar populations or dust content. Evidence of a disk is not readily apparent. Faint hints of disturbances can be observed in the surrounding halo, however it isn't clear if these are due to interactions or tidal effects. There does not seem to be evidence of any major ongoing merging activity.
