The galaxy presents as a spiral type, exhibiting a central bulge with moderate prominence. Faint spiral arms appear to extend outward from the bulge, indicating ongoing star formation within the galactic disc. The orientation of the galaxy allows a face-on view, enabling observation of its spiral structure. A bar feature appears present across the galactic center. There is no evidence of substantial merger activity or tidal disruption. The galaxy displays a mix of smooth light distribution, potentially indicative of an older stellar population, and regions with some texture, hinting at younger star clusters.
