The galaxy presents as a largely featureless, elliptical morphology. It appears to be generally smooth and rounded, with a slightly elongated, in-between shape. There is a central concentration of light, suggesting a dense nucleus or core region. The color profile exhibits a yellow-red hue, potentially indicative of an older stellar population. There is no evident spiral arm structure, dust lanes, or significant tidal disturbance in this image. Faint traces of a slight disturbance may be present, but they are difficult to resolve. The galaxy does not appear to be actively merging, though interactions cannot be completely ruled out. Overall, the observed characteristics suggest a mature, relatively quiescent elliptical galaxy.
