The galaxy exhibits a prominent disk structure, viewed at a slight angle from face-on. There are faint, but clearly discernible, spiral arm structures extending from the central bulge. The arms appear somewhat patchy, with regions of enhanced star formation indicated by a bluer hue. The central bulge displays a moderate size relative to the disk, and appears more yellow-white in color, suggesting an older stellar population. No strong bar feature is immediately obvious, though a subtle asymmetry in the central region cannot be ruled out. The overall morphology suggests a relatively normal spiral galaxy, with some indication of ongoing, albeit perhaps not intense, star formation within the spiral arms. There is a chance of it being in the early stages of minor merging or experiencing some kind of gravitational disturbance, but this is hard to know for sure. The light emitted suggests a medium sized galaxy.
