The galaxy presents as a centrally concentrated object with a generally smooth morphology. The shape is primarily round, with a slight deviation from perfect circularity. Light distribution is not uniform, it has a bright central core which seems to fade gradually towards the edges. There's a hint of a feature to the west, though that might be noise. Given the light profile and shape, it most likely belongs to the elliptical galaxy class. There is no strong evidence of spiral arm structure within the resolution of this image. Light emitted is mostly in the blue-green spectrum. There is no strong morphological evidence of ongoing or recent major merger activity. There might be signs of minor tidal disturbances or other unusual activity in the outer regions, though they would need to be confirmed with additional data.
