The observed galaxy presents as a prominent spiral structure. The arms are tightly wound, tracing a delicate and somewhat irregular pattern outward from the central bulge. The central region exhibits a bright and diffuse glow, suggestive of a concentrated stellar population. A subtle bar-like structure may exist within the bulge region, though its presence is not definitive. The spiral arms display a mottled texture, indicating regions of active star formation. The overall disk orientation is viewed nearly face-on, allowing for a clear view of its spiral morphology.
