The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a dominant, smooth bulge component. It is elliptical in shape, but does not appear perfectly spherical. Faint spiral arms are potentially present, but are difficult to resolve. The galaxy does not show any obvious signs of active galactic nuclei activity or a major merger event, although there may be minor disturbances in the outer regions. The color suggests a moderate amount of star formation, although it appears to be dominated by an older stellar population. Based on the size of this object, it is likely a moderately sized galaxy.
