The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting an elliptical morphology. There is a distinct color gradient, with the core appearing more yellow-orange, suggesting a higher concentration of older stellar populations or dust obscuration. The outer regions of the galaxy transition to a slightly bluer hue, possibly indicating the presence of younger stars, although this is less pronounced. The overall shape is elongated, with the major axis significantly exceeding the minor axis, lending a cigar-like appearance to the galaxy. There is no immediately obvious evidence of spiral arms or strong disk features. Subtle asymmetries or minor disturbances are present, but they are not significant enough to classify this as a major merger or strongly interacting system. The galaxy is not perfectly round but instead is an intermediate elliptical type.
