The observed galaxy presents as a spiral morphology, displaying a prominent disk structure. Two spiral arms appear dominant, exhibiting a medium winding. A bar structure is evident bisecting the central bulge. The bulge appears small relative to the overall disk size. No significant tidal distortions or signs of a major merger are immediately apparent, although some minor disturbances cannot be ruled out. The disk component shows a mottled texture, suggesting a degree of heterogeneity in stellar populations or dust distribution.
