This galaxy appears to be a spiral galaxy, though the disk is not face-on but appears to be at an angle to our line of sight. The galaxy exhibits a central bulge that appears largely smooth and contains the highest concentration of light and appears yellow in color. The spiral arms appear somewhat disrupted, with segments of blue color in the spiral arms. These areas of blue may suggest active star formation regions. The overall structure suggests a disk-dominated galaxy, but has a central bulge. There is a faint plume or tidal tail to the bottom of the galaxy, suggesting a past interaction with another galaxy. Based on the light distribution, the majority of the galaxy's stellar mass is concentrated in the central regions. There's a notable color gradient moving outwards from the center, transitioning from yellow to blue. This indicates a change in stellar populations, with younger, bluer stars more prevalent in the outer regions, and older, redder stars dominating the core.
