The galaxy presents as a face-on spiral with a prominent central bulge that displays a yellowish hue, suggesting an older stellar population. Spiral arms extend outwards from the bulge. These arms are tightly wound, exhibiting a blue tint indicative of ongoing star formation, although they may appear slightly diffuse. There is an absence of a strong bar feature bisecting the central bulge. The galaxy displays a relatively smooth disk component with minor asymmetrical features, possibly caused by minor gravitational interactions. There may be a slight warp on the outer edges.
