The galaxy presents as a centrally concentrated spheroid with a smooth luminosity profile. There is a distinct core region with a reddish-orange hue that gradually transitions to a cooler bluish-green in the outer regions. It's overall appearance is predominantly smooth with slight evidence of a very subtle disk component, but no distinct spiral arm features are visible. The shape appears largely elliptical, suggesting a minor degree of flattening. No major mergers or significant tidal disturbances are immediately apparent, although there may be evidence of minor distortions or interactions in the extended halo. It is a relatively high-mass galaxy with a moderate star formation rate.
