The galaxy presents as a relatively smooth, elliptical-like structure. Its color profile suggests a population of older stars with a redder hue dominating the central regions. There is some evidence of tidal disruption and merging in the form of a secondary concentration of stellar mass separated from the main body, hinting at a possible interaction with a smaller galactic body. The overall morphology indicates a system that is in a relatively advanced stage of merging and dynamical relaxation. There is little sign of ongoing star formation, with no prominent blue regions or HII emissions visible. The galaxy exhibits a generally concentrated light profile, with the highest intensity located in the center. A small amount of irregularity is observed in the outer regions. 
