The galaxy presents as a spiral type, exhibiting a central bulge with moderately wound spiral arms. The bulge appears a yellowish hue, suggestive of an older stellar population. The spiral arms are bluer in color, indicating regions of active star formation. There is evidence of patchy star formation, with discernible HII regions scattered along the arms. The galaxy is neither perfectly face-on nor edge-on, possessing a slightly tilted orientation relative to the observer. A faint bar structure might be present, but this is uncertain given the image resolution. There are no visible signs of major mergers or significant tidal disturbances, however minor interactions or disturbances are possible.
