The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that appears to be yellow. This suggests an older stellar population with a less active star formation rate. The shape is generally ellipsoidal, with a slight elongation, neither perfectly spherical nor highly flattened. There is no apparent spiral structure, nor any signs of significant tidal disturbances or ongoing mergers. Based on the observed color gradient and lack of distinct features, the galaxy appears to be a quiescent system without prominent dust lanes or bright star-forming regions. The outer regions display a gradual decrease in brightness, fading into the background sky, as well as a faint blue tinge around the outer edges.
