The galaxy presents as a largely smooth, elliptical or lenticular structure. It exhibits a concentrated central bulge, characterized by a bright, almost uniform yellow-white color. Radiating outward from the core, a fainter halo or disk-like component is visible. There is minimal evidence of well-defined spiral arms or significant dust lanes. The overall color profile suggests a relatively evolved stellar population, with a potential presence of ongoing, low-level star formation. While generally smooth, subtle variations in the outer regions hint at minor disturbances or interactions in its past. The overall shape appears more in between a perfect circle or a cigar shape. There appears to be no merging activity.
