The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, generally featureless morphology, though there are suggestions of subtle irregularities. The central region shows a bright, relatively compact core, gradually fading outwards. The isophotes appear elongated, deviating slightly from a perfectly circular shape. There is a minimal presence of blue light, suggesting a generally older stellar population. Evidence of ongoing star formation is not obviously apparent, but cannot be completely ruled out. Overall, the galaxy gives the impression of a system that is relatively evolved and undisturbed.
