The galaxy presents a generally smooth appearance with a discernible central bulge that dominates the overall light profile. The morphology suggests an elliptical type, however, the slight asymmetry and faint color variation hint towards the possibility of a disk component. The galaxy exhibits a reddish hue in the central region, potentially indicating an older stellar population. There might be a faint disk or spiral structure barely visible around the central bulge, as there is a slight flattening along one axis. There are potential signs of minor tidal disturbances or interactions, as seen through slight asymmetric features. The galaxy exhibits a small amount of blue light emission, which suggest the presence of some active regions of star formation. 
