The galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy. There are no prominent spiral arms visible. The object exhibits a fairly concentrated central bulge which fades gradually into a more diffuse halo. The galaxy has a somewhat elliptical shape, leaning more toward 'in-between' rather than perfectly round. There may be slight disturbances in the outer regions, but no major signs of an ongoing merger are apparent. Star formation activity is low based on the color profile, with a general blueish tint in the central region. Overall, the morphology suggests a relatively evolved system with a relatively low rate of star formation.
