The galaxy presents as a spiral type, viewed at an angle slightly offset from face-on. A prominent central bulge is visible, exhibiting a bright, yellowish-white hue. Spiral arms emanate from the central region, showing a bluer tint indicating the likely presence of younger, hotter stars. The arms appear somewhat diffuse and loosely wound. There is a possible minor disturbance in the arm structure, hinting at tidal interactions or a recent merger event. The overall morphology suggests a galaxy of intermediate mass with a relatively low star formation rate. The galaxy's shape is neither perfectly round nor elongated, and the light distribution gradually decreases from the center outward.
