The galaxy presents as a relatively compact and centrally concentrated object. Its overall form is smooth and elliptical in appearance, with a high degree of central symmetry. A faint, diffuse halo surrounds a brighter, more distinct core, fading gradually into the background. There is little evidence of spiral arm structure or significant dust lanes. Color gradients are subtle; the central region may exhibit a slightly redder hue relative to the outer regions, suggestive of an older stellar population. No apparent signs of ongoing major merging events are present, although some minor asymmetry cannot be ruled out at this image resolution. Based on its morphology, it appears to be a mature galaxy.
