The galaxy appears as a single, relatively smooth object with a high degree of central concentration. The color profile suggests a dominant population of older stars, exhibiting a reddish-yellow hue. There is a lack of prominent spiral arms or distinct features indicative of active star formation. The galaxy appears to be generally spheroidal in shape, approaching circularity. There is no clear evidence of ongoing mergers or significant tidal disturbances. The overall structure points towards a mature, relatively undisturbed galaxy.
