The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, diffuse light distribution. It appears generally rounded in shape with a minor asymmetry, potentially indicating past or ongoing interaction. The central region shows a concentration of yellow light, which may be indicative of an older stellar population. The outer regions display a bluer color, possibly signaling the presence of younger stars or regions of active star formation. The overall morphology suggests a significant spheroidal component with minimal visible spiral structure. There is a slight warping or minor disturbance, but overall the galaxy appears relatively undisturbed.
