This galaxy, observed at a redshift of approximately 0.12, presents a primarily smooth, elliptical morphology. It exhibits a luminous central bulge, suggesting a concentration of older stellar populations. The outer regions of the galaxy appear less defined, fading gradually into the background sky. There is a slight elongation, deviating somewhat from a perfectly circular shape. The galaxy appears relatively undisturbed, lacking any obvious signs of tidal interactions or major mergers. A subtle color gradient is present, with the central region displaying a bluer hue compared to the redder outer halo, possibly indicating ongoing, albeit limited, star formation in the core.
