The galaxy presents a largely smooth morphology, appearing as a concentrated, ellipsoidal structure. Its light profile suggests a significant bulge component, exhibiting a centrally concentrated brightness that gradually diminishes outwards. There is little evidence of distinct spiral arms or prominent star-forming regions. The galaxy's color is predominantly yellow-red, implying an older stellar population and a relatively low rate of ongoing star formation. Slight irregularities or disturbances in its outer regions point to possible minor interactions or past merger events. The overall impression is that of a massive, evolved galaxy residing at a considerable distance.
