The galaxy presents as a moderately luminous, compact object with a relatively smooth morphology. It exhibits a slightly elongated, elliptical shape. The color profile suggests a redder central region, potentially indicating an older stellar population concentrated toward the galactic nucleus. The outskirts appear slightly bluer, hinting at the presence of younger, star-forming regions or a population gradient. There is some faint indication of possible tidal disturbances or asymmetric features, but these are subtle and may warrant further investigation to determine if they are intrinsic to the galaxy or due to projection effects or minor interactions. A more complete assessment would require higher resolution imaging and spectroscopic analysis.
