The galaxy presents as a lenticular or early-type spiral galaxy viewed at an oblique angle. The central bulge is prominent, exhibiting a smooth, concentrated light profile with a yellowish hue, suggesting an older stellar population. Faint, diffuse disk-like features extend from the bulge, exhibiting a bluer color, likely indicating the presence of younger stars and regions of on-going star formation. The disk does not display well-defined spiral arms or significant dust lanes. The overall morphology suggests a relatively evolved galaxy with a dominant bulge component. There does not appear to be any nearby merger events.