The galaxy presents as an elliptical or lenticular type, appearing largely smooth with no prominent spiral arm structures visible. Its overall shape is somewhat elongated, but generally rounded with a slight flattening. A brighter, more concentrated central region, possibly a bulge, is apparent, surrounded by a more diffuse halo. The galaxy exhibits a color gradient, with the central bulge appearing redder or yellower than the outer regions which trend towards bluer hues. This may indicate an older stellar population concentrated in the center and some ongoing star formation in the outskirts. There is a possible hint of a minor disturbance or asymmetry in the outer disk on one side.
