The galaxy presents a distinct spiral morphology with prominent arms. These arms exhibit a moderate winding, neither tightly coiled nor loosely extended. They appear somewhat flocculent in nature. The bulge component is moderately sized, not dominating the disk but certainly noticeable. There is a hint of a bar-like structure extending from the central bulge, although it does not appear very strong or well-defined. The galaxy's disk is not perfectly face-on, appearing tilted relative to our line of sight. There is evidence of ongoing star formation within the spiral arms, as indicated by the presence of regions exhibiting a bluer hue. These regions are interspersed with older stellar populations, giving the galaxy a multi-colored appearance in its arms. The overall impression is that of a relatively undisturbed spiral galaxy, though there are signs of minor disturbances present within the arm structure possibly from interactions.
