The galaxy presents as a moderately bright, irregular structure exhibiting a diffuse morphology. A central, brighter region is apparent, surrounded by a less defined, extended halo. The light distribution suggests a complex system, potentially undergoing interactions or displaying significant star formation activity. Patches of bluer light are observable within the central region and along the edges, indicative of younger stellar populations and ongoing star formation. Some tidal features may be visible. The galaxy lacks a clear spiral arm structure, which would make it an irregular galaxy. There is an apparent non-uniformity in the color distribution across the galaxy. Redder hues are present in the areas of what appear to be dust lanes. These are indicative of older stellar populations or dust obscuration. Overall, the galaxy presents a dynamic and relatively unorganized appearance.
