The galaxy exhibits a generally smooth morphology with some discernible features. It appears to be neither perfectly round nor highly elongated, presenting an intermediate shape. While the galaxy's structure is mostly undisturbed, there are hints of minor disturbances potentially arising from tidal interactions or internal dynamics. There may be a merging event occurring with a dwarf galaxy or stellar stream, seen by the lopsidedness in the halo. The color gradients suggest varying stellar populations across the galaxy. The central region shows a higher concentration of light with a bluer tinge. It will be beneficial to explore additional spectral data for a robust conclusion.
