The galaxy presents as a barred spiral type, viewed at an angle, possibly inclined roughly 25 to 40 degrees from edge-on. A prominent, elongated central bulge dominates the visual appearance, with a high degree of concentration towards the galactic center. The bulge exhibits a yellowish hue, suggesting a population of older stars. Fainter spiral arms emanate from the ends of the bar structure. These arms appear relatively smooth, rather than displaying significant knotty or clumpy structures indicative of active star formation regions, they are more tightly wound. The overall color of the spiral arms is slightly bluer compared to the bulge, pointing to the presence of younger stars. The galaxy's outer regions are diffuse, lacking a sharply defined edge. There are no apparent signs of major mergers or significant tidal disturbances in the overall morphology.
