The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish hue, which likely indicates an older stellar population. The overall shape is mostly round and there does not appear to be a disk structure. Faint and fuzzy extension with a redder color is visible around the central bulge. There is no evidence of spiral arms or dust lanes. It shows no strong indication of ongoing merger activity or significant disturbances in its structure. Based on the red color, the light is likely redshifted. Given its smooth and round structure, it might be classified as an elliptical galaxy, potentially of type E0-E3 on the Hubble sequence.
