The galaxy presents as a centrally concentrated, elliptical-like morphology. It exhibits a smooth light distribution with no readily discernible spiral arm structure or prominent dust lanes. The color profile transitions from a yellowish-white core to a redder, more diffuse outer halo. There are no signs of strong tidal interactions or recent merger events, based on the absence of extended tidal tails or irregular morphological features. The galaxy appears largely undisturbed with what seems to be a fairly evolved stellar population.
