The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light distribution. The galaxy exhibits a yellow-orange hue, suggesting a stellar population dominated by older, redder stars with suppressed recent star formation. The galaxy's shape is approximately spheroidal, showing only slight deviations from perfect circularity. There is a possible indication of a minor disturbance or interaction, suggested by subtle asymmetries in its overall structure. The galaxy's visual appearance suggests it is relatively massive. The galaxy is not actively undergoing a major merger, however, there may be slight irregularities present.
