The galaxy presents a generally smooth, elliptical morphology. There is a high degree of central concentration. The galaxy exhibits a yellowish-white core, transitioning outwards to a less distinct halo, with faint extensions. There is an absence of any clear spiral arm structure or dust lanes. The color suggests an older stellar population. The overall round shape and lack of significant tidal features suggests it has not experienced any recent major mergers, although there may be minor disturbances visible in the faint extensions. The object appears relatively isolated in the image.
