The galaxy presents as a moderately bright object with an elliptical morphology. The light distribution appears relatively smooth, with no prominent spiral arm structures or distinct features visible. The galaxy exhibits a color gradient, with the central region appearing more yellowish, potentially indicating an older stellar population, while the outer regions have a slightly bluer hue suggesting the presence of younger stars or ongoing star formation. There appears to be a minor interaction or disturbance within the system. The galaxy is neither perfectly round nor elongated but displays a morphology in between. The galaxy's appearance does not suggest a major ongoing merger, but the possibility of a minor interaction or past merger event cannot be ruled out. 
