The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a general elliptical morphology, appearing mostly round but with some deviation. There may be signs of minor disturbances in its structure, potentially indicative of past interactions or mergers, but this is not conclusive from the image. There is no prominent disk structure detected. The color gradient is subtle, with a slightly redder core transitioning to a bluer outer halo. The galaxy shows little evidence of active star formation.
