The galaxy presents as a somewhat diffuse and elongated structure. Its overall color appears to be slightly reddish, suggesting an older stellar population. There is little evidence of distinct spiral arms or a prominent bulge. The light distribution is relatively smooth, with some subtle clumping of light visible toward the central region. While there is no clear sign of a recent major merger event, some slight asymmetry in the light distribution hints at potential minor gravitational interactions or past disturbances. There does not appear to be an extremely active region of star formation. 
