The galaxy presents a generally smooth morphology, appearing largely featureless in the available image. Its shape is somewhat elongated, deviating slightly from a perfect circular profile. The color distribution is not uniform; the central region exhibits a concentration of yellow light, suggesting an older stellar population. There is a subtle gradient towards slightly bluer hues in the outer regions, possibly indicating the presence of younger stars, although star formation appears to be low overall. The overall appearance indicates a galaxy that is likely elliptical or lenticular in form. There is no obvious evidence of a major ongoing merger, although the possibility of past minor disturbances cannot be entirely ruled out.
