The galaxy appears as an elongated, cigar-shaped structure, suggesting it is an elliptical galaxy viewed at an oblique angle or a lenticular galaxy. The central region exhibits a higher surface brightness and a yellowish-white hue, likely indicating an older stellar population. Moving outwards from the center, the brightness decreases, and the color shifts to a slightly bluer tone. This may indicate the presence of younger stars or some ongoing star formation in the outer regions, although it is not prominent. There is a slight asymmetry in the galaxy's outer regions. The galaxy exhibits a smooth appearance overall, with no clear evidence of spiral arms or significant dust lanes. There may be a very faint, diffuse halo surrounding the main body of the galaxy. The overall morphology suggests a system that has undergone significant dynamical relaxation.
