This galaxy presents as a disk-shaped structure, viewed nearly edge-on. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older, redder stars. The disk shows a distinct blue color, particularly towards the outer edges, indicating ongoing star formation within spiral arms. The galaxy displays some features that suggest gravitational disturbances, possibly indicating interactions with other galaxies. There is evidence of a merger, though it appears to be in its early stages. There is a slight degree of asymmetry, suggesting an active or recent merger event. Overall, the system exhibits a mix of older stellar populations in the bulge and younger, star-forming regions within the disk.