The galaxy presents a predominantly smooth morphology. The overall shape appears elliptical, exhibiting a moderate degree of roundness. There is some evidence of a possible minor disturbance or interaction, though a significant portion of the classification votes indicate no merging or major disturbance. The color profile suggests a population of relatively older stars, with a lower rate of star formation based on its redder color. A minor merger cannot be ruled out however, based on the dual nature of the core. The redshift data reveals that this galaxy is at a considerable distance from our own, so it is likely to have a very massive center. 
