The galaxy presents as a somewhat irregular, diffuse structure. There is evidence of disturbed morphology, possibly resulting from minor gravitational interactions or internal dynamics. A central, somewhat brighter region is apparent, potentially indicating a nucleus. The overall color is consistent with an intermediate redshift of 0.21, with an apparent mix of stellar populations ranging from aged to newly formed. The galaxy's angular size suggests a substantial physical extent, approximately 10.9 kiloparsecs, further supporting the observation of internal structure. The galaxy appears to have a complex formation history with indications of star formation.
