The galaxy presents as a moderately sized, lenticular or early-type spiral system, exhibiting a dominant central bulge. This bulge appears to be relatively smooth and luminous, indicating an older stellar population and a concentration of mass. A faint, flattened disk is visible surrounding the bulge, albeit with low surface brightness. The disk shows hints of spiral arm structure, but these features are poorly defined. The overall color of the galaxy suggests a redder spectrum, consistent with a lower rate of star formation. There is a slight possible minor disturbance, possibly due to an ongoing or past minor merger event. No tidal tails or extended halos are clearly discernable.
