The galaxy presents an elongated shape, likely a disk galaxy viewed at an oblique angle. There appears to be a bright central bulge or core, emitting a significant amount of light. The galaxy's color profile shows a mixture of wavelengths, with a concentration of blue light toward the central regions and hints of green and red further out along its edges. This suggests ongoing star formation, particularly within the central region. The galaxy appears relatively undisturbed, showing no major signs of recent or ongoing mergers. However, there may be some minor internal disturbance visible in the image. The luminosity is very strong, potentially indicating a high density of stars within the galaxy. The overall structure appears relatively smooth.
