The galaxy presents as a face-on spiral with a prominent, luminous central bulge. This bulge appears to be a mix of older stellar populations, judging by its yellowish-white hue. A distinct bar-like structure bisects the bulge, appearing rather strong and extending into the inner regions of the spiral arms. Two well-defined spiral arms emanate from the ends of the bar. These arms appear tightly wound around the bulge, with a structure that seems to be composed of many stars and gas clouds, displaying faint blue regions along the arms, indicating ongoing star formation. The overall form exhibits a degree of symmetry, though the spiral arm structure appears slightly flocculent. There are no obvious signs of a major merger or significant tidal disruption. A smaller bulge is present, suggesting the galaxy is not an elliptical galaxy. The galaxy appears to be relatively isolated.
