The galaxy presents as a luminous, elliptical-like structure with a smooth, concentrated central bulge. Its overall shape is relatively undisturbed, showing no signs of a major merger, although some minor asymmetry or a slight tidal interaction might be present. The galaxy exhibits a yellow-ish hue, indicating a population of older stars, and a lower rate of active star formation. The radial profile suggests a gradual decrease in luminosity from the center outwards. It has an estimated radius of roughly 2.2 kpc, making it a dwarf galaxy.

