The galaxy presents as a slightly inclined disk galaxy, exhibiting a somewhat smooth morphology with subtle features. The central bulge appears prominent and exhibits a yellowish-orange hue, possibly indicative of an older stellar population. Moving outwards from the bulge, a faint, bluish disk structure is observed, suggesting the presence of younger, hotter stars and potential ongoing star formation, although the star formation rate is relatively low for a galaxy of its size. There is no obvious indication of a major merger event. Faint, diffuse spiral arm structures can be observed, but the overall structure seems somewhat disordered. The galaxy appears relatively isolated.
