The galaxy presents a generally smooth morphology, suggestive of an elliptical galaxy. There is some asymmetry, with a slight extension in one direction. There are no immediately obvious spiral arms or a distinct disk structure. Its light profile appears centrally concentrated with a relatively rapid fall-off in brightness. Faint color gradients are present across the galaxy, potentially indicating variations in stellar populations or dust content, or some features within the galaxy. I do see signs of a possible minor disturbance or a possible minor merger event, as evidenced by the slight asymmetry, but more data would be needed to confirm.
