The galaxy presents as a lenticular or possibly a spiral galaxy viewed at a significant angle to its plane. A bright, concentrated central bulge is apparent. The disk exhibits a yellowish-orange hue, suggestive of an older stellar population with relatively low current star formation. Faint spiral arm structures may be present, though the resolution is insufficient for definitive identification. There is some visual indication of potential tidal interactions or minor disturbances present. The galaxy appears moderately smooth.
