The galaxy presents as a face-on spiral, exhibiting well-defined spiral arms. These arms are tightly wound, initiating near the central bulge and extending outwards. The bulge appears relatively small and concentrated, exhibiting a yellowish hue indicative of an older stellar population. Patches of blue coloration can be seen along the spiral arms suggesting areas of active star formation. The overall morphology does not show strong evidence of recent major merging events or significant tidal disturbances.
