The galaxy appears as a somewhat symmetrical, diffuse object with a prominent central bulge. The light distribution suggests a smooth profile, transitioning gradually from a bright, concentrated core outwards. There is some indication of an extended, fainter halo surrounding the core. The color is primarily bluish-white, indicative of a moderate to high stellar temperature, which is consistent with ongoing star formation. Subtle hints of a disk-like structure are visible, though the overall morphology appears dominated by the bulge. A slight asymmetry in the outer regions could suggest a minor interaction or disturbance, but the overall appearance is relatively undisturbed. There may be indications of low-level merging or tidal features but the galaxy remains largely intact.
