The galaxy appears to be a relatively small, low-mass system with a faint, diffuse morphology. The overall color suggests a mix of stellar populations, with a subtle blue hue indicating the presence of some young, hot stars, but also significant contribution from older, redder stars. There is a hint of spiral structure or some other form of internal organization, but it is not clearly defined. Some areas of the galaxy appear more disturbed and clumpy than others, potentially indicating ongoing or recent interactions or minor mergers. Overall, the galaxy appears to be a relatively quiescent, low star-forming system.
