This galaxy appears to be a relatively compact object with a dominant central bulge region exhibiting high surface brightness. The overall morphology suggests a possible disk galaxy, but the disk is not well-defined. There is some distortion in the arms, it's possible that the galaxy is currently undergoing a minor interaction with a smaller galaxy or has experienced one in the recent past. The color gradients indicate an active star formation with bluer regions suggesting the presence of younger stellar populations, contrasted by more central redder areas that likely contain older stars. The galaxy is not perfectly symmetrical, and shows signs of irregularity in its shape, possibly related to the aforementioned interaction.
