The galaxy presents a generally smooth morphology, displaying a concentrated central bulge with a discernible disk component. The disk appears relatively compact. The color distribution suggests a possible ongoing interaction or recent merger event, characterized by regions of increased blue luminosity that may signify zones of enhanced star formation. Overall, the galaxy's structure implies an evolutionary stage where disk formation is either ongoing or has been recently perturbed, potentially influencing the distribution of stellar populations and the galaxy's color gradients. There appears to be a faint hint of tidal tails suggesting some kind of disturbance, though it is very faint and needs further investigation. 
