The galaxy presents as an elliptical morphology, with a smooth, relatively featureless profile. The light distribution appears concentrated towards the center, indicating a prominent bulge. It exhibits an elongated shape, neither perfectly spherical nor highly flattened. There is a discernible color gradient, shifting from a yellowish hue at the central region to a redder tone in the outer regions. This suggests an older stellar population dominates, particularly away from the core, with minimal ongoing star formation. Minor disturbances in the morphology are possibly present, but further investigation is needed. No clear signs of a major merger event are immediately apparent.
