The galaxy presents as a relatively smooth, single object. It appears to be elliptical in shape, lacking any distinct spiral arm structure or features. The color profile suggests the galaxy is primarily composed of older stellar populations, with a noticeable lack of bright blue regions indicative of active star formation. The concentration of light is highest at the galaxy's center, gradually fading towards the edges. There is no indication of significant tidal disturbances or merging activity. The galaxy's overall appearance suggests it is a mature, relatively quiescent system.
