The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile. The core region displays a distinct yellowish-orange hue, suggesting an older stellar population with relatively low levels of ongoing star formation. The galaxy appears to have a moderate mass. The outer regions exhibit a fainter, more diffuse halo of light, blending gradually into the background sky. There is no clear evidence of spiral arms or significant dust lanes. The overall structure shows no obvious signs of a major merger event, although a subtle asymmetry might indicate a minor interaction in its past. Its shape can be described as somewhere between round and elongated.
