The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a generally round morphology, though with a slight elongation. The galaxy appears bluish in color, indicating the presence of some younger stellar populations, but also with some redder components toward the core. There is no readily apparent spiral structure or prominent disk. The light distribution appears fairly uniform, with a gradual decrease in intensity from the center outwards. No major mergers or strong tidal disturbances are visible, suggesting a relatively undisturbed evolutionary history, though possibly a minor disturbance. The galaxy exhibits an absolute magnitude suggesting it is dwarf sized. Based on the galaxy's apparent color and morphology, star formation rates are expected to be low.
