The galaxy presents as a somewhat elongated, lenticular or edge-on spiral type. The light distribution appears relatively smooth, with a central bulge that dominates the overall brightness. There is a faint suggestion of a disk component, though it appears to be viewed at a high inclination, making detailed structural analysis difficult. The galaxy exhibits a reddish hue, which implies a stellar population that is somewhat older. There is some evidence of a minor gravitational disturbance, but no clear indication of a major merger event.
