The galaxy presents as a lenticular or early-type spiral galaxy. Its overall morphology is characterized by a prominent bulge that appears relatively smooth and centrally concentrated. Surrounding the bulge is a fainter, diffuse disk. Although subtle, there are hints of spiral structure within the disk.

The color gradient suggests a higher concentration of older stellar populations within the bulge, and somewhat younger populations in the disk. There is no evidence of intense star formation regions. The galaxy seems to be relatively isolated, with no signs of major mergers or tidal disturbances, though the disk could be slightly warped.
