The galaxy presents as a largely smooth, elliptical morphology, elongated along a single axis. The light distribution is concentrated towards the core, with a noticeable decrease in luminosity moving towards the outer regions. The color profile suggests a relatively evolved stellar population, trending toward redder hues. There is no discernible spiral structure or significant dust lane obscuration. The galaxy appears relatively undisturbed, without any major signs of tidal features or ongoing mergers.
