This galaxy appears to be relatively smooth in morphology. The central region exhibits a concentrated, bright, and yellowish light profile, suggesting an older stellar population. Fainter, bluer light is observed on the left side of the galaxy, showing evidence of some disk-like or irregular structure. It may be undergoing minor disturbances, hinting at possible past interactions or internal processes affecting its morphology, but it doesn't seem to show any ongoing merger events, although it is slightly asymmetrical. The galaxy exhibits an elliptical shape, leaning towards roundness, with a slight elongation.
