This galaxy exhibits a morphology suggesting ongoing or recent interaction. A dominant central bulge is visible, appearing yellowish, indicative of an older stellar population. A fainter, bluer region extends from the central bulge, possibly a tidal tail or a region of enhanced star formation triggered by the interaction. There is a clear disturbance in the morphology; the galaxy appears asymmetrical. Based on the colour and apparent shape, this galaxy may be undergoing a merger or close interaction with another galaxy, resulting in its distorted appearance. Overall, the galaxy exhibits a mix of evolved and younger stellar populations distributed in a disrupted structure.
