The galaxy presents a roughly elliptical morphology, appearing largely smooth in structure with a diffuse halo. The central region exhibits a moderate concentration of light, transitioning smoothly into the outer regions.  There is a slight indication of asymmetry or tidal feature on one side, suggesting a possible past interaction or minor disturbance. The color profile appears relatively uniform across the galaxy, with a subtle redder hue. This suggests a stellar population dominated by older stars and a low rate of on-going star formation. The overall form indicates a galaxy somewhere between a spiral and elliptical galaxy, possibly a lenticular. 
