The galaxy presents a generally smooth, elliptical morphology with an apparent lack of prominent spiral arms. Its overall structure appears largely spheroidal, though there are hints of a possible disk-like component. There is a central, brighter region suggestive of a galactic bulge. The galaxy's color is predominantly bluish-white in the central regions, possibly indicating a younger stellar population, with a faint reddening trend towards the outer edges. It appears as a relatively isolated system, with some evidence of minor disturbances or interactions, possibly hinting at past merger events.
