This galaxy exhibits a morphology characteristic of a spiral galaxy, though some disturbances are visible. The galaxy's structure is dominated by a distinct disk component with evidence of spiral arms. These arms appear moderately wound, with some portions difficult to discern. The central bulge appears relatively small in comparison to the disk, but it is still present. A hint of a bar can be observed across the central region, although it does not appear to be prominent. The color distribution shows a bluer component in the arms, suggesting recent or ongoing star formation, and a yellower/whiter central region that may indicate an older stellar population. Overall, there appears to be some degree of interaction or disturbance, resulting in the distortion and asymmetrical appearance of the spiral arms.
