This galaxy presents as a centrally concentrated, elliptical system, appearing largely smooth in texture, with a relatively high degree of rotational symmetry. It exhibits a bright, yellowish core that dominates the overall luminosity, suggesting an older stellar population. The luminosity smoothly decreases moving outward from the center. The overall color is redder than that of a typical spiral galaxy, consistent with evolved stars and minimal ongoing star formation. There is minimal evidence of distinct features like spiral arms or dust lanes; instead, the light appears relatively uniform, indicative of an early-type galaxy. There is a faint reddish hue in some of the outer regions of the galaxy. The lack of discernible structure implies a relaxed morphology, likely reflecting a history of mergers and/or the cessation of significant star formation.
