The galaxy presents as a somewhat diffuse object, appearing neither purely elliptical nor strongly spiral in morphology. A central bulge is subtly suggested, but without high resolution, distinct spiral arms are not definitively discernible. The overall light distribution is moderately centrally concentrated. There are some visual disturbances. It looks like there may be a merger event present. The light profile suggests a slightly elongated shape. Color gradients are visible with a slightly bluer hue in the outer regions compared to the central areas.
