The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated light profile, with a bright, well-defined core. Moving outwards from the center, the intensity gradually decreases without any distinct spiral arm structures or prominent dust lanes visible. There may be a slight extension of the galaxy along a particular axis; however, it is mostly round. The overall color suggests an older stellar population, with the light predominantly in the redder wavelengths. There is no evidence of active star formation regions or intense blue light from young stars. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal distortions in its morphology. There might be a nearby object that causes a minor disturbance.
