The galaxy presents as a somewhat diffuse, disk-like structure with an apparent inclination to our line of sight. Its overall color profile appears predominantly blue, suggesting a population of younger, hotter stars. There is evidence of a central, brighter region, possibly indicating the presence of a bulge or a concentration of stellar activity. Distinct features such as spiral arms are not clearly defined, which may be due to the image resolution, the galaxy's inherent morphology, or obscuration by dust. The galaxy appears to be undergoing some type of significant disturbance. This could involve the presence of tidal tails, distorted morphology, or any other indicator of gravitational interaction.