The galaxy appears to be a spiral galaxy, viewed at an oblique angle. The presence of spiral arms is indicated by faint, diffuse structures extending from the central bulge. The spiral arms appear somewhat tightly wound. The central bulge is prominent, exhibiting a smooth, concentrated distribution of light, suggesting an older stellar population. The disk component is evident, with bluer colors indicating regions of ongoing star formation. The overall color suggests the galaxy is in an intermediate stage of stellar population evolution, neither strongly blue indicating rapid star formation, nor uniformly red indicating a passive, evolved system. There may be a weak bar structure spanning the central region. No obvious signs of a major ongoing merger are visible, however, there are minor irregularities within the disk.
