The observed galaxy presents an elliptical morphology with notable disturbances. A bright central core is visible, surrounded by a diffuse halo. The light distribution within the halo appears asymmetric, suggestive of tidal interactions or recent accretion events. Patches of bluer light, likely indicating regions of active star formation, are interspersed across the body of the galaxy. Possible signs of a tidal tail or bridge extend outwards along one side, signifying a potential merger in progress. The overall structure indicates a galaxy undergoing some form of interaction or gravitational disturbance. The overall color of the galaxy appears relatively blue, hinting at a younger stellar population or ongoing starburst activity.
