The observed galaxy presents a distinct spiral morphology. The galaxy exhibits a prominent, moderately sized bulge that appears yellowish-white, indicating a concentration of older stellar populations. Two well-defined spiral arms emanate from the central bulge. These arms appear tightly wound. The disk is oriented face-on with some evidence of a bar feature. Patches of bluer regions are visible within the spiral arms, suggesting ongoing star formation activity. Overall, the galaxy's structure suggests a relatively massive system with an active period of star formation and a well-established disk component. The galaxy does not appear to be undergoing any major merging events, and it has a slightly dusty appearance.