The galaxy presents as a relatively compact object, exhibiting a generally smooth morphology. The primary color appears to be a light shade of blue, indicative of a younger stellar population and ongoing star formation, although there are redder areas in the center, which could indicate a population of older, redder stars or the presence of dust. The light is highly concentrated towards the center, suggesting a high degree of central mass concentration. There are also irregular spots in the galaxy which could be merger remnants. There is little evidence of spiral arms or a well-defined disk structure.
