The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its color profile suggests a relatively evolved stellar population, with a yellowish-red hue indicating older, cooler stars dominating the light output. There is a slight color gradient with the central region displaying a slightly more blue-green hue. This could be a combination of different star populations or an artifact of how the color image was created. There is no clear evidence of spiral arm structure or significant dust lanes. No signs of major mergers or strong tidal disturbances are apparent, although very minor irregularities cannot be ruled out at this resolution.
