The observed galaxy presents a somewhat amorphous structure, appearing relatively compact. A central, bright core is evident, suggestive of a concentration of stellar mass or potentially an active galactic nucleus. Diffuse, extended features surround this core, exhibiting an irregular morphology. These extensions display varying intensities, indicating possible uneven distribution of stellar populations or dust obscuration. There is an object of similar size nearby. The galaxy exhibits a color gradient, with the central regions appearing bluer, potentially indicating younger stellar populations or increased star formation activity compared to the more reddish outer regions. There is little evidence of well-defined spiral arms or a distinct disk structure. Subtle asymmetries in the galaxy's shape may point to past or ongoing interactions or merger events. The galaxy's overall structure suggests it may be an irregular or disturbed system, possibly undergoing evolutionary changes.
