The galaxy presents as a spiral type, exhibiting prominent spiral arms. These arms are not tightly wound, suggesting a later Hubble type, and are somewhat clumpy in appearance, with regions of bluer light indicative of on-going star formation. The central bulge is moderately sized and has a smooth, diffuse appearance, exhibiting a yellowish-white hue indicative of an older stellar population. Faint evidence of a bar structure is present, though it is not a dominant feature. There are signs of minor tidal disturbances or interactions, with some asymmetry in the outer regions, but no clear signs of a recent major merger event.
