The object appears to be a galaxy of moderate apparent size. It exhibits a non-uniform light distribution. The galaxy shows subtle visual features, possibly indicative of a disk-like structure or the presence of spiral arms that are difficult to discern due to the low fraction of smooth or featured components. The image shows characteristics that may indicate a merger event or tidal disturbances, likely from a minor disturbance or a merger interaction. There is also a low percentage of smooth features within the galaxy. The bluer color in the central region may indicate a higher concentration of younger, hotter stars, while the outer areas appear relatively redder, which would suggest an older stellar population.
