This galaxy presents as an elliptical or lenticular type, appearing predominantly smooth in structure with a slight elongation. Its central bulge exhibits a concentrated luminosity, transitioning smoothly outward to a less luminous halo. The color profile suggests an aging stellar population with a dominance of redder wavelengths, indicating minimal current star formation. Subtle disturbances, such as faint tidal features, are possibly present but are not overtly significant, thus suggesting that the object could have previously undergone a merger.
