The galaxy presents as a spiral type, viewed approximately face-on. It exhibits a distinct central bulge, surrounded by a relatively well-defined disk. The spiral arms appear tightly wound, displaying a symmetrical structure extending from the central bulge. There are indications of recent star formation within the spiral arms. The galaxy exhibits a bluish tint, suggesting the presence of a young stellar population. No significant signs of a major merger event or strong tidal disturbances are readily apparent. The galaxy displays a moderate amount of light concentration in the central regions, gradually decreasing towards the outer edges. The overall morphology suggests a relatively undisturbed and well-formed spiral galaxy.
