The observed galaxy appears to be undergoing significant interaction or disturbance. The central region exhibits a relatively compact, bright core suggesting a high concentration of stars. Surrounding this core, there are distinct tidal features. Faint, extended tails extend outward from the main body, indicating a possible gravitational interaction with another galaxy or a recent merger event. The overall morphology is irregular, lacking a clear spiral or elliptical structure. Patches of color variation are visible across the galaxy, potentially indicating regions of enhanced star formation. Specifically, the bright center indicates older stars whereas the cyan areas denote higher levels of star formation.
