The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, homogenous texture throughout the majority of its visible surface. The central region displays a higher concentration of light. Faint, diffuse extensions are observed at the far extents of the galaxy. There appears to be a slight elongation of the galaxy along one axis, giving it a somewhat cigar-shaped appearance. The galaxy presents a reddish hue, hinting at a population of older stars, indicating low recent star formation. There is no evidence of spiral arms or significant dust lanes. No major mergers or disturbances are apparent.
