The galaxy presents as a face-on spiral with a moderate bulge. Two distinct spiral arms emanate from the central region, exhibiting a medium winding pattern. Star formation appears to be actively occurring within these spiral arms, indicated by regions of bluer light. The overall disk component of the galaxy shows evidence of organized structure rather than being completely smooth. There is no significant indication of a strong bar feature bisecting the central bulge, nor is there evidence of any major mergers or tidal disturbances.
