The galaxy appears to be a spiral type, exhibiting distinct spiral arm structures. The arms are relatively tightly wound around a central bulge. There is a clear nucleus, which is quite prominent, yellow colored, and indicative of an older stellar population. The spiral arms exhibit a bluer hue, suggesting the presence of younger, hotter stars and ongoing star formation. There is no apparent bar structure present in the central region. The galaxy displays a generally undisturbed morphology, with no signs of major merging activity. The spiral arms seem symmetric. There is a color gradient going from the center (yellow/orange) to the outer parts of the disk (blue). The size of the bulge with respect to the galaxy disk is small to moderate. Overall, the galaxy presents a well-defined spiral structure.