The galaxy appears as an elliptical structure with a prominent central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a bluish tint, possibly indicating the presence of younger stars and ongoing star formation. The galaxy is elongated, with an axis ratio indicating it is not perfectly circular but rather somewhat flattened. There is a slight distortion in its shape, hinting at a possible past interaction or merger event. The overall morphology is generally smooth, with a lack of distinct spiral arms or prominent dust lanes.
