This galaxy presents an irregular morphology, with noticeable deviations from a perfect elliptical or spiral structure. A central, bright, and relatively compact region of high luminosity is visible, suggesting a concentrated nucleus or core. The color profile indicates a blue-white center transitioning to more green hues in the outer regions, possibly indicative of varying stellar populations. A distinct, albeit small, disturbed feature is apparent on one side of the galaxy, suggesting either an ongoing minor interaction with a smaller object or internal instability. Overall, this galaxy appears to be actively evolving, potentially through mergers or internal star formation processes, leading to the observed asymmetrical features and color variations.
