The galaxy appears as a relatively smooth and concentrated object, characterized by an elliptical morphology. There is a bright, centrally located bulge exhibiting high surface brightness. The galaxy displays a redder color profile, suggestive of an older stellar population. No prominent spiral arm structures or significant dust lanes are visible, leading to the characterization as likely an elliptical galaxy. There is an apparent lack of substantial star formation occurring within the galaxy. The overall light distribution is centrally concentrated, with the intensity gradually decreasing towards the outer regions of the galaxy. The isophotes appear to be closely aligned, which would indicate the galaxy is highly elliptical in shape.
