The galaxy presents as a generally smooth, elliptical object, exhibiting a gradual increase in luminosity towards the core. The central region is highly luminous, exhibiting a bright, concentrated nucleus. The color profile suggests a relatively homogeneous stellar population across the visible extent of the galaxy, with the dominant hue tending towards blue-green. There is a slight indication of disturbance in the structure. It may be an indication of minor tidal distortion, potentially resulting from a gravitational interaction or merger event. However, the dominant visual impression is that of a fairly undisturbed and centrally concentrated system.
