The galaxy exhibits a predominantly smooth morphology, with a high degree of central concentration. The light distribution suggests an elliptical-like structure. The galaxy is mostly rounded, but displays some deviation. There is no clear evidence of spiral arms or a distinct disk structure. The color gradient indicates a redder central region which may represent an older stellar population compared to bluer outer edges. No prominent tidal features or indications of a major ongoing merger are discernible, though some minor disturbances cannot be ruled out.
