The galaxy presents as a somewhat amorphous, moderately luminous object with a relatively smooth appearance. It exhibits a slightly elongated shape, deviating from a perfectly circular morphology. The central region appears brighter and more concentrated. There is some evidence of structural features, possibly indicative of a disk component, although these features are not sharply defined. Hints of possible ongoing or past interactions with neighboring galaxies are present. The color profile suggests a mix of stellar populations, with some regions exhibiting bluer hues consistent with ongoing star formation.
