The galaxy presents as a relatively compact, elliptical-like structure. It appears largely smooth in texture, with a high degree of central concentration. The color profile suggests a moderately evolved stellar population, exhibiting a yellowish-orange hue. No distinct spiral arms or prominent dust lanes are discernible. The overall morphology indicates a system that has likely undergone significant dynamical relaxation, potentially representing an early-type galaxy. The absence of significant tidal features suggests it is not currently undergoing a major merger event, although the possibility of past minor interactions cannot be ruled out. Overall the galaxy seems generally uninteresting.
