The galaxy presents as a spiral structure with a moderately sized central bulge. A bright, nearly elliptical core region transitions into a diffuse disk. Two distinct spiral arms are visible, originating near the ends of the core region and wrapping outwards in a somewhat broken pattern. These arms exhibit areas of higher luminosity, possibly indicating regions of active star formation. There is a potential weak bar structure spanning across the core, though obscured by the intensity of the core luminosity. The disk component appears relatively undisturbed. There is no significant evidence of a major merger event but there is likely some kind of disturbance. The overall color is relatively even throughout. The galaxy is not seen edge-on.
