This galaxy appears to be a disk galaxy, viewed at an oblique angle. There is evidence of a central bulge that exhibits a yellowish color, suggesting an older stellar population. The disk itself displays a bluer hue, indicating ongoing star formation. The morphology appears disturbed, showing evidence of a possible merger event or tidal interaction on one side, with diffuse light extending away from the primary galactic structure. The overall shape is somewhat elongated, with an approximate apparent size indicative of a relatively large physical size, and a significant stellar mass. The colors suggest a moderate star formation rate, but a low specific star formation rate.
