The galaxy presents as a spiral type, viewed at an intermediate angle. The central bulge exhibits a smooth, concentrated light distribution, appearing bright white. The spiral arms are moderately defined and display a clumpy structure with areas of active star formation, indicated by a blueish hue throughout the arms. Patches of dark dust and gas are also visible within the arms, contributing to their irregular appearance. There is a subtle indication of interaction with another galaxy or gravitational disturbance on the right side of the image. The galaxy does not appear to be perfectly symmetrical; the shape of the arms and the distribution of star-forming regions are not uniform. The overall color suggests a mix of stellar populations, with older stars contributing to the yellowish light from the bulge, and younger, hotter stars responsible for the bluer regions within the arms. 
