The galaxy presents as an elliptical morphology, appearing largely smooth in structure with a concentrated central bulge. There is a slight elongation, although it is mostly round. The galaxy displays a color gradient, with a yellowish-orange hue dominating the central region, suggesting an older stellar population. Outer regions appear slightly bluer, potentially indicating more recent star formation, though this is not readily apparent in the image. There is no obvious evidence of spiral arms or a prominent disk structure. Subtle irregularities might suggest minor gravitational interactions or disturbances. The galaxy appears relatively isolated without obvious major merging companions.
