The galaxy appears to be a relatively bright elliptical type, with a smooth, diffuse morphology dominating the central region. The core exhibits a yellowish-white hue, indicating a likely older stellar population. Fainter, reddish emissions are present in a horizontal distribution across the galaxy, possibly indicative of dust lanes or regions of ongoing or recent star formation, though the smoothness suggests a less prominent disk structure. There are minor irregularities in the galaxy's morphology, potentially hinting at past interactions or minor disturbances. The overall shape is mostly circular, with only a slight elongation along one axis.