The galaxy appears as a yellowish-white, relatively smooth object with a concentrated central bulge. Its shape is approximately elliptical, with a moderate degree of roundness. There is no visible evidence of spiral arms or a prominent disk structure. The galaxy's light distribution suggests a well-mixed stellar population with a dominant older population, as indicated by its color. There is no strong indication of ongoing major merging events or significant disturbances, though some minor irregularities in the outer regions cannot be ruled out. The general morphology suggests that it is likely an elliptical galaxy with minimal recent star formation activity.
