The galaxy presents as a spiral type, exhibiting a relatively face-on orientation with a notable central bulge. Spiral arms are visible, displaying a loosely wound structure. The arms show signs of active star formation, indicated by the bluish hue, suggesting a population of young, hot stars. A bar structure is also apparent, running through the central region of the galaxy. The bulge appears moderately sized, with a yellowish color indicative of an older stellar population. No significant signs of major mergers or tidal disturbances are immediately apparent. Overall, the galaxy exhibits characteristics consistent with a barred spiral galaxy undergoing active, but not extreme, star formation.
