The galaxy appears as a centrally concentrated, fairly symmetrical object. Its morphology can be described as smooth and elliptical, with a round shape. There is no apparent disk structure or spiral arm morphology visible in this image. There is no visual evidence of major merger activity, but it is possible there are minor disturbances. Overall, it appears to be a relatively isolated system, with a red color implying an older stellar population. Based on the color profile and lack of distinguishing structures, this appears to be an early-type galaxy undergoing low levels of star formation.
