The galaxy presents as a spiral type, oriented at a moderate inclination relative to the observer. Its morphology appears to be dominated by a large, moderately luminous bulge, concentrated towards the galactic center. Faint spiral arms are present. These arms appear somewhat tightly wound around the central bulge, with an ambiguous arm count due to image quality. The color profile suggests a population of older stars in the bulge, indicated by the yellow hue. Star formation appears to be very minimal, indicated by the lack of prominent blue regions associated with young, hot stars. The overall structure is relatively undisturbed, showing no signs of major mergers or significant tidal interactions with neighboring galaxies. There may be a weak bar-like structure. The disk appears relatively smooth, lacking prominent dust lanes.
