The galaxy presents as a centrally concentrated spheroid, generally smooth in appearance. It exhibits a somewhat elliptical morphology, with a moderate ellipticity. There's no readily discernible spiral arm structure or a pronounced disk component visible in the image. The galaxy appears to be dominated by a central bulge, with a radial color gradient suggesting a centrally concentrated stellar population that may be older than its outer regions. Faint extensions can be seen implying slight tidal disturbances. The overall color index suggests moderate star formation, but it is not dominated by hot, young stars. No ongoing major merger activity is apparent, but some minor disturbance cannot be ruled out.
