The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. Coloration suggests an older stellar population, with a yellowish hue dominating the core and inner regions. There is a lack of discernible spiral arm structure or dust lanes. The galaxy appears to have a relatively regular, rounded morphology with no obvious signs of major tidal disturbances or recent major mergers. There is an apparent lack of intense star formation, and is more consistent with a passive or quiescent galaxy.