The object presents as a spiral galaxy, viewed at a moderate inclination. The central bulge appears prominent and elongated along the major axis, displaying a yellowish hue indicative of an older stellar population. Two distinct spiral arms emanate from the central region, exhibiting a tightly wound morphology. These arms are traced by regions of blueish light suggesting ongoing star formation. Evidence of a bar structure across the bulge seems to be in place, as the bulge is clearly elongated. The overall structure indicates no major merger or significant tidal disturbances, although there might be very minor disturbances.
