The galaxy presents a moderately luminous profile, characterized by a relatively smooth, centralized light distribution. The overall shape appears to be largely elliptical, tending toward round rather than elongated. There may be a hint of a disk structure. The central region is significantly brighter, indicative of a concentrated nucleus, possibly hosting a supermassive black hole. There may be evidence of minor gravitational disturbances. The galaxy exhibits colors consistent with moderate star formation.
