The galaxy presents as a centrally concentrated object with a diffuse and somewhat amorphous structure extending outwards. It is relatively compact, but not perfectly spherical, with a suggestion of some extended features or irregularities. The color profile suggests a mix of stellar populations. The central region appears yellowish, potentially indicating older, more evolved stars. Surrounding this, a bluer hue is observed, which could indicate the presence of younger, hotter stars or ongoing star formation. There seems to be some subtle hints of disturbance, although a clear merger is not obvious. The galaxy exhibits a moderate level of star formation. Overall, the galaxy does not appear to be a pure elliptical, nor a well-defined spiral; it likely is a transitionary galaxy.
