The galaxy presents a generally smooth morphology with a relatively high degree of roundness. There is some indication of disturbance or possible merging activity in the image. The galaxy exhibits a color gradient, with a more yellow-orange hue concentrated in the central region, potentially indicating an older stellar population. A bluer, less concentrated region is also visible, possibly suggesting a younger population of stars or ongoing star formation. Overall, the galaxy's light distribution is somewhat concentrated toward the center, although not perfectly spherical. It also seems there is a small object in the vicinity which might be a smaller galaxy that is undergoing a merger.
