The galaxy presents an elliptical morphology, displaying a smooth, centrally concentrated light distribution. The core region exhibits a yellowish-white hue, possibly indicative of an older stellar population. Moving outwards from the core, the galaxy shows a subtle transition to a slightly bluer color. The disk appears elongated, with an estimated axis ratio suggesting a moderately inclined viewing angle. No prominent spiral arm structures or dust lanes are discernible. The overall light profile appears relatively smooth, without significant irregularities or distortions. The galaxy does not appear to be undergoing any major merging events, though some minor disturbances cannot be ruled out.