The galaxy presents as a moderately luminous, isolated system. It has a smooth, elliptical morphology and exhibits a generally featureless appearance, lacking prominent spiral arms or a distinct bar structure. The galaxy's color profile suggests a relatively evolved stellar population, with a dominant reddish hue in the central region transitioning to slightly bluer tones towards the outer edges. There is a subtle asymmetry in the color distribution, hinting at potential variations in stellar populations or dust content across the galaxy. The apparent lack of significant morphological disturbances suggests that it is a relatively relaxed system, potentially having undergone past merging activity but now largely settled. The overall appearance indicates a galaxy with a low rate of ongoing star formation.
