The galaxy presents as a moderately sized, well-defined structure, exhibiting a shape between elliptical and spiral. Its central region appears smooth and concentrated, suggesting a prominent bulge. The outer regions display subtle features, possibly faint spiral arms or a disk-like component. There is a mild asymmetry, indicating potential gravitational interaction or past merging events. The galaxy appears to be actively forming stars with moderate levels. The color gradient suggests a higher concentration of older stellar populations in the core, transitioning to younger, bluer stars in the outer regions. There are hints of minor disturbances or tidal features, suggesting ongoing or recent interaction with another galaxy. The overall visual impression is of a galaxy undergoing a dynamic evolutionary stage.
