The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile exhibits a centrally concentrated core, surrounded by a more diffuse halo. The core region appears to be a bluish-white hue, suggesting the presence of a younger stellar population, or higher star forming region. The outer regions seem redder in comparison. There is a slight suggestion of a disk-like structure, but it is not prominent. There is some low-level asymmetry or disturbance visible in the outer regions. This could be an indication of minor interaction or past merger event.
