The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bulge with a yellowish-white hue, suggesting an older stellar population. The light distribution appears quite symmetrical with a gradual falloff in intensity from the core to the outer regions. There is little evidence of spiral arms or significant dust lanes. The galaxy displays a fairly regular, rounded shape with a slight deviation from perfect circularity. There does not appear to be any obvious signs of ongoing or recent major merging activity. The galaxy's overall color gradient suggests that star formation is either suppressed or has largely ceased within its main body. Based on the observed characteristics, this galaxy is likely a quiescent, early-type system.
