The galaxy presents as a fairly symmetrical, elliptical-like structure with a concentrated central bulge. The light distribution appears smooth and centrally concentrated. The galaxy exhibits a noticeable color gradient, transitioning from a slightly bluer hue in the outer regions to a redder, more yellow color toward the core. This suggests a differential stellar population, with potentially younger, bluer stars in the outer parts and older, redder stars dominating the central region. There are no obvious signs of spiral arms or a prominent disk structure. The morphology indicates the galaxy is undisturbed, displaying no significant signs of recent mergers or tidal interactions. There is a hint of fuzziness or extended emission surrounding the main body of the galaxy, possibly indicating a faint stellar halo. The relatively red color suggests a moderate redshift, placing it at a considerable distance. Overall, the morphology is consistent with that of an early-type galaxy.
