The galaxy presents as an elliptical morphology, though with some possible deviations from perfect symmetry. The light distribution appears concentrated towards the center, indicating a prominent bulge. There is some evidence of a faint extended halo or envelope surrounding the central region. Some subtle distortions are observable in the outer regions, suggesting gravitational interaction. The overall color suggests an older stellar population, potentially with minimal ongoing star formation, which is consistent with an elliptical galaxy classification. There is also a suggestion of a faint tidal feature.
