The galaxy presents a primarily face-on orientation, exhibiting a prominent disk structure. Distinct spiral arms emanate from the central region, displaying a moderate winding pattern. The bulge appears relatively substantial in size, with a noticeable bar feature extending across the core. The colour gradient suggests an active star formation, with a yellowish-red hue prominent toward the core, possibly indicative of an older stellar population, with bluer regions apparent in some of the spiral arms, indicating regions of younger stars. There is no obvious indication of major mergers or significant tidal disturbances, the outer disk appears relatively undisturbed.
