The galaxy presents as an elliptical or lenticular type, displaying a smooth, concentrated luminosity profile indicative of an older stellar population. The object exhibits a moderate degree of ellipticity; appearing cigar shaped. There is a noticeable central bulge, though precise structural details are difficult to resolve. A very small fraction of features point to minor disturbances or merging activity. Based on its colour and shape, the galaxy likely has a moderately high mass and low star formation rate.
