The galaxy presents as a lenticular or edge-on spiral type, exhibiting a noticeably elongated shape. Its color profile appears primarily reddish-yellow, suggesting an older stellar population with a lower rate of ongoing star formation. There is some evidence of a central bulge, as indicated by a slight concentration of light, but distinct spiral arm structures are not readily apparent, possibly due to the viewing angle or intrinsic properties of the galaxy. No signs of recent or major merger events are visible; the galaxy appears relatively undisturbed. Overall, it seems to be a quiescent galaxy undergoing minimal star formation with a significant red shift.
