The galaxy presents as a centrally concentrated system with a smooth, somewhat elliptical morphology. There is a high likelihood it is an elliptical galaxy. The object's core exhibits a notable concentration of light, transitioning into a more diffuse halo. The color profile suggests an evolved stellar population, trending towards redder hues. No distinct spiral arms or significant dust lanes are discernible, and the object presents with a relatively smooth texture, although there are hints of minor disturbances in the outer regions. It appears to be a quite massive galaxy, and it presents weak evidence of ongoing star formation. Some merging activity or tidal interactions with companion galaxies may be present, but not strongly apparent. The object is moderately rounded in shape, and shows some evidence of being more elongated.
