The galaxy appears to be a relatively smooth, elliptical galaxy with a slight elongation. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population. A faint, bluish halo surrounds the central region, possibly representing younger stars or some residual star formation. There is no clear evidence of spiral arms or prominent dust lanes. The overall structure suggests a system that is not currently undergoing significant merging activity, though some minor disturbance cannot be ruled out. The galaxy displays a relatively compact appearance.
