The galaxy presents a disk-like morphology, though not clearly defined, and is observed face-on. The central region exhibits a higher surface brightness, suggesting the presence of a bulge, albeit not a prominent one. Traces of spiral arm structure are faintly visible, with bluer colors indicating regions of ongoing star formation along these arms. The overall color of the galaxy appears relatively blue, indicative of a younger stellar population and active star formation. The disk appears somewhat disturbed or irregular, possibly due to interactions or internal processes. There are indications of tidal features or merging activity with an interaction disturbance. There appears to be an absence of a strong central bar.
