The galaxy presents as a smooth, elliptical structure. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue, suggesting an older stellar population. Fainter, greenish-blue light surrounds the central bulge, potentially indicating the presence of younger stars and some on-going star formation, particularly in the outer regions. The galaxy's overall shape is mildly elongated, but the structure shows no signs of strong tidal distortions, major mergers, or significant dust lanes. A small amount of minor disturbance is possible but is not readily apparent.
