The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable central bulge. Its overall shape is elongated, suggesting a non-circular morphology, with an approximate axis ratio of about 0.6. There is a slight color gradient observed, with the central region appearing more yellowish and the outer regions exhibiting a bluer hue. No distinct spiral arm structures are apparent. The galaxy appears to be a relatively isolated system, without any signs of major interaction or ongoing mergers. The surface brightness distribution indicates a gradual decline from the core outwards, which further implies a single, unified structure. Its size appears small, with an effective radius on the order of 1.4 kpc, typical of a dwarf galaxy.
