The galaxy presents as a spiral morphology, observed at a moderate inclination relative to our line of sight. The galactic bulge appears prominent, with a bright, concentrated central region, likely indicative of an older stellar population. Faint spiral arms extend outwards from the central bulge. These arms appear relatively tightly wound, exhibiting distinct star-forming regions characterized by a bluer hue. There is a possibility of a weak bar structure, with a slight elongation observed across the central bulge. The overall color profile suggests an active star formation rate.
