The galaxy presents as a spiral galaxy, with a clearly defined disk structure. Two prominent spiral arms emanate from a central bulge. The bulge appears moderately sized, with a yellow hue suggesting an older stellar population. The spiral arms exhibit a blue tint, indicative of ongoing star formation. The arms are tightly wound close to the bulge, opening into a medium winding pattern as they extend outwards. There is no clear indication of a bar feature bisecting the central bulge. The morphology suggests no significant recent merger events, although there may be a minor disturbance on the upper part of the galaxy.
