The galaxy presents as a centrally concentrated object with a diffuse, elliptical morphology. A smooth overall appearance dominates, with a high degree of central light concentration. The color profile suggests a bluer core region, likely indicating recent or ongoing star formation. Moving outwards, the color shifts toward a redder hue, possibly reflecting an older stellar population. The overall structure appears relatively undisturbed, with no clear signs of tidal tails, strong asymmetries, or major merger events. A minor irregularity is suspected on one side, possibly indicating a weak gravitational interaction or minor disturbance.
