The galaxy appears to be relatively small in angular size. Its overall morphology is difficult to classify definitively, however, it is likely a disturbed system, as there are some hints of asymmetry and irregular features, possibly indicating a recent or ongoing interaction or merger. The galaxy's light profile seems concentrated with a slightly elongated or disturbed shape. There is an indication of a minor tidal disturbance or faint extended features in the galaxy's halo. The color profile suggests a mix of stellar populations, with some bluer regions, potentially indicating younger stars or star formation activity, and redder regions associated with older stellar populations. Overall, the galaxy presents characteristics suggestive of a dynamically active system.
