The galaxy appears as a moderately bright, centrally concentrated object. It exhibits a somewhat smooth morphology, although there are hints of features that could be described as either a disk-like structure or minor disturbances in its shape. The central region presents an orange hue, which may indicate an older stellar population. Surrounding this central region is a more diffuse, fainter halo or outer disk with a slightly bluer color, potentially indicating ongoing or recent star formation. Overall, the galaxy has a nearly round appearance, but with some irregularity to its edges. There is no strong evidence of a major ongoing merger, though the potential for minor tidal interactions cannot be ruled out based on the observed morphology alone.
