The galaxy appears to be undergoing an interaction or merger. The primary body displays a somewhat amorphous shape, with a central bright core. Hints of bluer light are visible within the main body, which is indicative of possible ongoing star formation. There are also redder components or potential tidal tails/features extending from the main body. These features are indicative of older stellar populations. Overall, the galaxy does not present a well-defined spiral or elliptical structure; instead, it exhibits a more irregular and disturbed morphology.