The galaxy presents as a diffuse, yellowish-white object. Its overall morphology is somewhat ambiguous due to its smooth appearance and lack of well-defined spiral arms or a prominent central bulge. The light distribution suggests a relatively even spread of stars across the galaxy's body. There are subtle hints of clumpy substructures or regions of higher stellar density within the galaxy's disk, potentially indicating areas of active star formation or the presence of unresolved satellite galaxies. There appears to be minor asymmetry in its overall shape which could be indicative of tidal interactions or an ongoing merger event with a smaller companion galaxy. The outer regions exhibit a gradual fading of light intensity, suggesting a less densely populated stellar halo.
