This galaxy exhibits a generally smooth morphology. The object appears elliptical with an intermediate axis ratio, exhibiting a moderate degree of elongation. Its color profile suggests an older stellar population, with a central bulge that shows a distinct reddish-yellow hue, indicative of evolved stars. A fainter, bluer halo surrounds the bulge, suggesting the presence of some younger stars. There are no obvious signs of strong spiral arm structures or active star formation, though a slight blueness in the outer regions hints at a low level of ongoing stellar birth. There is no obvious strong gravitational distortion or evidence of a recent major merger event. Minor disturbances cannot be ruled out. The galaxy's apparent size is relatively small, consistent with a distant object.