The galaxy presents a morphology consistent with a spiral type, exhibiting a defined, though not highly pronounced, spiral arm structure. The central bulge appears relatively small compared to the overall disk size. A prominent bar-like structure traverses the galactic center. The disk shows a mixture of resolved and unresolved components, hinting at both ongoing star formation regions and a more diffuse stellar population. There is evidence of minor disturbances, possibly due to an interaction, indicated by slight asymmetry in the arm structure. The colour index suggests a range of stellar ages, with bluer regions indicating younger stars and star formation, and yellower regions indicating older stellar populations. Overall, it is a face-on galaxy of a middling size that appears barred, and with a small, but possibly active, bulge.