The galaxy presents a generally smooth morphology, appearing largely featureless in this observation. Its shape is approximately elliptical, exhibiting a high degree of roundness. The central region appears brighter and more concentrated, gradually fading into the surrounding halo. There is a subtle color gradient, with a slightly bluer hue in the outer regions compared to the somewhat redder central bulge. No evidence of spiral arms, bars, or significant dust lanes are discernible. There are no obvious signs of ongoing major mergers or tidal disturbances. The overall appearance suggests a galaxy with a relatively evolved stellar population.
