The galaxy presents an overall smooth morphology, with a bright central region suggesting a concentration of stellar mass. Its shape appears to be somewhere between round and elliptical. There are hints of potential disturbances in its structure, possibly indicating minor interactions or past merger events. Star formation appears to be present but not dominant, with a bluer color in certain regions hinting at ongoing or recent star formation activity. Given the color gradients and indications of some structural irregularities, this galaxy appears to be in a transitional phase of its evolution.
