The galaxy presents as a spiral type, exhibiting a prominent central bulge and a well-defined, although somewhat patchy, disk. Two spiral arms are clearly visible, emanating from the ends of a strong central bar. These spiral arms are tightly wound. The bulge appears moderately large and dominates the inner regions of the galaxy. The color profile suggests an older stellar population concentrated in the bulge, indicated by the yellowish hue. Star formation seems to be ongoing within the disk, as indicated by the bluer regions within the spiral arms. There is no obvious evidence of a major merger, although some minor disturbances within the arms cannot be ruled out.
