The galaxy presents a mostly smooth morphology, with a shape that is neither perfectly round nor highly elongated. The light profile appears centrally concentrated, suggesting a lack of prominent spiral arms or significant disk features. The galaxy exhibits a color gradient, with the central region appearing more yellowish-white, potentially indicating an older stellar population or a higher concentration of dust. The outer regions display a bluer hue, possibly associated with younger stars or a less dusty environment. There is no strong evidence of ongoing major merger activity, although some minor asymmetries or disturbances cannot be entirely ruled out. Overall, the galaxy appears to be a relatively quiescent system, characterized by a primarily smooth, centrally concentrated light distribution and a moderate color gradient.
