The galaxy presents as a slightly elongated, lenticular or early-type spiral galaxy. There is a smooth appearance to the galaxy, although some subtle features are visible. The galaxy appears largely featureless, with a dominant central bulge. There is a slight hint of a disk structure.

Based on the color profile, the galaxy appears to be composed primarily of older stars, with a redder hue evident across the structure. The star formation rate appears to be low. There is no indication of major interactions or recent merger events. 
