This galaxy presents a face-on spiral morphology. The central bulge appears moderately sized, exhibiting a yellowish hue, suggestive of an older stellar population. Prominent spiral arms extend outwards from the central bulge, displaying a defined, multi-armed structure. The arms appear tightly wound closer to the bulge. Some spiral arm structures exhibit distinct segments, possibly indicating areas of increased star formation activity.

A subtle bar structure may be present, though not a particularly strong feature. The disk exhibits a generally smooth texture with a slight blue tint, suggesting a presence of younger stars and on-going star formation. There does not seem to be any clear indication of a major merger event, though some minor disturbances or tidal features may be present in the outer regions.
