The galaxy presents an overall elliptical morphology, though it does not appear perfectly spherical, exhibiting a slightly elongated shape. The central region displays a concentrated luminosity, indicating a significant stellar population and potentially a supermassive black hole actively accreting material. The color gradient transitions from a yellowish core to a redder halo. The smooth light distribution suggests that the galaxy has largely completed its major mergers, with no large scale disturbances or tidal features visible. Based on its apparent color and overall morphology, it is likely composed predominantly of older stellar populations, with a relatively low rate of ongoing star formation.
