This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, exhibiting a yellow hue, indicative of an older stellar population. No distinct spiral arms or prominent dust lanes are discernible. The galaxy is neither perfectly round nor highly elongated, appearing more elongated in shape. There is no obvious indication of ongoing major mergers or significant tidal disturbances, although there is faint, amorphous light surrounding the primary body. The overall structure suggests a galaxy that has undergone significant merging in the past, resulting in the relaxed, elliptical morphology observed.
