This galaxy appears to be a relatively large, luminous object, likely a massive elliptical or lenticular galaxy. It exhibits a centrally concentrated morphology, with a smooth, diffuse light distribution, and there is no evidence of prominent spiral arms or a well-defined disk structure. The galaxy's color gradients suggest a higher concentration of older stellar populations in the core, grading to slightly bluer, possibly younger populations in the outer regions. There is a suggestion of ongoing star formation. Its overall shape is more rounded than elongated. The galaxy does not appear to be significantly disturbed or undergoing a major merger, though there is a slight asymmetry suggesting it is not perfectly relaxed.
