The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. It displays a generally round morphology, though a slight elongation is discernable. The galaxy exhibits a dominant bluish-white hue concentrated in the central region, suggesting the presence of a population of hot, young stars within that area or a possible active galactic nucleus. Fainter, more diffuse yellow and red colors are observed in the outer regions of the galaxy, possibly indicating an older stellar population and the presence of dust. Subtle indications of minor disturbances or tidal features can be seen, though the overall structure remains largely undisturbed.
