The galaxy presents as an elongated, diffuse object with a somewhat disturbed morphology. The overall color is bluish, suggesting the presence of younger, hotter stars. There is a noticeable irregularity in the light distribution; one region is significantly brighter and more concentrated than the rest of the galaxy. This brighter region may indicate an area of intense star formation or possibly a galactic nucleus. The remaining structure exhibits a fainter, more spread-out luminosity profile, hinting at a possible tidal interaction or ongoing merger event. Overall, the galaxy appears to be undergoing some form of dynamic process.
