The galaxy presents as a spiral galaxy, observed at an inclined angle. The central bulge appears moderate in size and exhibits a yellowish hue, likely indicating an older stellar population. Two prominent spiral arms emanate from the central region. The arms are relatively well-defined and possess a moderately wound morphology. The arms appear bluish, suggesting active star formation. There appear to be no signs of major disturbances or a recent merger event, the galaxy seems to be isolated with no clear indications of a galactic bar. Some regions along the spiral arms exhibit clumpy structures, which are likely HII regions, and some appear to be areas of ongoing star formation.
