The galaxy appears as a single, relatively smooth object with a slightly elongated shape. The color profile shows a broad spectrum, indicating a mix of stellar populations. The overall color is slightly blue-green in the center, which may suggest active star formation. The outer regions appear somewhat redder, potentially indicating an older stellar population or dust extinction. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy does not appear to be undergoing any major mergers or interactions, though there might be a minor disturbance in its shape. Its features are smooth, and the elongation may suggest a transition between elliptical and lenticular.
