The galaxy presents a primarily smooth morphology, suggesting a relatively evolved system. There appears to be a distinct central bulge region that exhibits a yellow-orange hue, potentially indicating an older stellar population. The outer regions of the galaxy fade gradually into the background sky, with a bluer tint compared to the core. The overall shape is roughly elliptical, showing a moderate degree of ellipticity but with some evidence of a disk-like structure. There are no obvious signs of strong tidal interactions or major disturbances, implying that it is currently a relatively isolated and undisturbed system. Subtle asymmetries may hint at minor past interactions, but the dominant impression is that of a well-formed, fairly quiescent galaxy.
