The galaxy presents as a lenticular or early-type spiral galaxy, with a smooth, centrally concentrated bulge and a faint disk. The bulge exhibits a slightly elliptical morphology. The disk component is significantly fainter and appears truncated with hints of spiral structure. The galaxy is oriented at a high inclination relative to our line of sight. The overall color is relatively red, suggesting an older stellar population with limited ongoing star formation. There is no clear evidence of a recent major merger or strong tidal interaction based on the galaxy's morphology.
