The galaxy exhibits a primarily smooth morphology. The light distribution suggests a centrally concentrated spheroid with a high degree of rotational symmetry, appearing largely circular in projection. There is a suggestion of a diffuse, extended halo surrounding the brighter central region. The color profile appears to be relatively uniform across the galaxy, with a slight reddening towards the center and bluer tones in the outer edges. No prominent spiral arm structures or dust lanes are discernible, and no obvious signs of recent major merger events are present. There is some indication of minor tidal features, possibly suggesting past minor interactions or accretion events. The galaxy has an estimated mass of 10^10 to 10^11 solar masses. Star formation is observed, but it is low.
