The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. Its overall shape is somewhere between round and elongated, appearing as a flattened spheroid. There's a subtle color gradient, with the central region exhibiting a slightly bluer hue compared to the outer edges. The outer regions show subtle irregular features, possibly faint tidal tails or distortions, suggesting past or ongoing gravitational interactions with another galaxy. There is no clear evidence of well-defined spiral arms or a prominent disk structure. The galaxy exhibits a low star formation rate, indicating it is primarily composed of older stellar populations. There are no clear indications of a recent major merger, but minor disturbances and distortions are present.
