The galaxy presents as a relatively smooth, rounded structure. There is a concentrated central bulge that appears yellowish-white, possibly indicating an older stellar population. A very faint, diffuse disk-like structure surrounds this bulge. There appears to be little to no evidence of spiral arm structure or active star formation regions within the disk. There does not seem to be any signs of tidal disturbances or ongoing merging activity within the galaxy. The overall morphology suggests an elliptical or lenticular galaxy, likely with a substantial stellar mass.
