The galaxy appears as a single, relatively smooth object with an elliptical morphology. The central region exhibits a higher concentration of light, appearing a yellow-orange hue, suggesting an older stellar population. The outer regions of the galaxy appear to gradually fade into the background sky, with a slightly more greenish color, potentially indicating the presence of younger stars or ionized gas. The galaxy shows no strong evidence of spiral arms or significant dust lanes. There is no obvious active galactic nucleus. There is no morphological evidence of a major merger occurring, though minor disturbances cannot be excluded at this resolution. The overall round appearance suggests it may be close to an E0.
