The galaxy presents a somewhat irregular morphology, not clearly elliptical or spiral. It exhibits a diffuse, nebulous structure with hints of clumpy features. The central region appears slightly more concentrated, with a subtle color gradient suggesting potential variations in stellar populations. There is evidence of disturbances, possibly indicative of past or ongoing interactions or mergers. Overall, the galaxy appears to be a mid-sized object with faint, diffuse features. The light distribution indicates a galaxy that has some star formation but also has regions where star formation might be slowing down.
