The galaxy exhibits an irregular morphology, appearing to be in a state of interaction or disturbance. A central, concentrated region of high luminosity is apparent, likely representing a galactic nucleus or a region of intense star formation. Emanating from this central area is an extended, fainter structure that shows evidence of tidal features or disrupted spiral arms. The color profile is suggestive of ongoing star formation, with bluer hues observed in the extended structure, potentially indicative of younger stellar populations. Overall, the galaxy does not appear to have a well-defined disk or elliptical shape and lacks any prominent features, it rather shows signs of a potentially recent or ongoing merger or interaction.
