The galaxy presents as an elliptical morphology, appearing largely smooth and concentrated towards the center. There is a noticeable absence of spiral arms or a distinct disk structure. The central bulge appears bright and somewhat spheroidal, exhibiting a yellowish-white hue, possibly indicating an older stellar population. The outer regions of the galaxy gradually fade in intensity, exhibiting a more diffuse and somewhat reddish color. The overall structure suggests a relatively evolved system with minimal ongoing star formation, consistent with an early-type galaxy classification. The lack of significant dust lanes or tidal features suggests the galaxy is not undergoing any major merging events or active gravitational interactions.
