The galaxy presents a clear spiral structure, with well-defined arms emanating from a central bulge. The arms display a moderately wound morphology, suggestive of an intermediate spiral type. Star formation appears active throughout the disk, particularly along the spiral arms, indicated by the patchy distribution of bluer regions. The central bulge exhibits a yellowish hue, possibly indicating an older stellar population. There is no clear indication of a strong bar structure, and the bulge size is moderate. The overall structure shows some signs of disturbance, but the image suggests the disturbance is relatively minor, with no clear major merging event readily apparent. The disk is oriented somewhat face-on, allowing for the detailed observation of its spiral features.
