This galaxy exhibits a relatively smooth morphology, appearing as an elliptical galaxy with a slightly elongated shape. The light distribution is centrally concentrated, with a bright core that gradually fades outwards. The outer regions are less defined, suggesting a diffuse stellar halo. There is minimal evidence of spiral arm structure or distinct dust lanes, lending credence to its classification as an elliptical galaxy. The overall color profile appears to be relatively uniform, with a subtle shift towards redder hues, indicating an older stellar population. There is no apparent evidence of significant ongoing star formation from the image alone.
