The galaxy presents as a lenticular or early-type spiral with a relatively smooth and concentrated morphology. The overall shape is somewhat elongated, exhibiting an intermediate axis ratio that is neither perfectly round nor highly elongated. There are some hints of disk-like structures, but overall the light distribution is centrally concentrated and has little or no spiral arm structure. The galaxy appears generally homogenous in color, with a slight bluer hue than expected, which may indicate low levels of on-going star formation, even though the morphology is not that of a star-forming galaxy. There are no obvious signs of major mergers or tidal disturbances that would indicate recent interactions.
