The galaxy presents a prominent, well-defined spiral structure. The spiral arms are somewhat flocculent and extend noticeably from a central bulge. The bulge appears moderate in size, contributing significantly to the overall luminosity of the galaxy but not dominating its structure. Patches of intense star formation are visible within the spiral arms, characterized by a bluer hue, indicating the presence of young, hot stars. The disk appears relatively thin. There is a suggestion of a bar feature bisecting the central bulge along its major axis. The overall morphology suggests a relatively undisturbed system, with no clear signs of major ongoing merger activity or tidal distortions.
