The galaxy presents a morphology indicative of a relatively smooth structure. The light distribution suggests a central bulge surrounded by a disk that is not clearly resolved. There is a hint of some disturbance in the outer disk, but the galaxy does not appear to be undergoing a major merger. The overall shape leans towards being in between round and cigar-shaped. The redder color suggests a population dominated by older stars. Based on these characteristics, the galaxy is likely a relatively massive system with a moderate rate of star formation.
