The galaxy presents a flattened, elliptical morphology. A central, bright core is visible, surrounded by a more diffuse halo. The galaxy's color appears to trend from bluer hues in the inner region to slightly redder tones in the outer halo. No prominent spiral arms or dust lanes are discernible, indicating it is likely not a spiral galaxy. There is no indication of a major ongoing merger, although some minor irregularities in the halo suggest the possibility of past interactions. The shape seems to be quite round, with the ratio of minor to major axis diameter just above 0.8. The Sersic index is approximately 1, suggesting the light distribution is moderately centrally concentrated. Overall, the galaxy appears to be a relatively smooth, elliptical system.