The galaxy presents as a relatively smooth, elliptical-like structure. There is a central, bright core, likely a dense concentration of stars. Fainter, diffuse light extends outwards from the core, forming a somewhat elongated shape. The gradient of light intensity decreases gradually from the core to the outer edges. Slight bluer hues may indicate pockets of star formation. There is no clear evidence of spiral arms or a distinct disk structure. Possible disturbances in the symmetry of the outer regions, but no obvious signs of a major merger event.
