The galaxy presents a generally smooth morphology with a slight asymmetry. The central region appears as a bright, concentrated core, potentially indicating a significant concentration of stars or an active galactic nucleus. A less distinct extension emanates from the core. This extension exhibits a slightly elongated shape and a yellowish color compared to the bluer hue observed in the central region. This color difference may signify variations in stellar populations or dust distribution. The galaxy's overall structure shows no clear spiral arm features or a well-defined disk, suggesting it is likely an elliptical or lenticular galaxy undergoing a potential merging event. There are also faint signs of possible tidal disruptions, but the data is not definitive.
