The galaxy presents as a smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish-white hue, suggesting an older stellar population. Fainter, diffuse material extends outwards from the core, with a slight elongation along a major axis. There is no visible evidence of spiral arms, dust lanes, or active star-forming regions within the optical spectrum. The overall color is indicative of a relatively quiescent system with a low star formation rate. There does not appear to be any evidence of recent mergers or tidal disturbances. 
