The galaxy presents as a largely featureless, smooth, elliptical-like structure. Its overall shape is consistent with a spheroid, exhibiting a high degree of roundness. The central region displays a concentrated luminosity, appearing significantly brighter and more yellowish than the surrounding halo. There is no discernable disk component or spiral arm structure. No evidence of major or minor mergers is detected. The galaxy's morphology suggests a classification towards the early-type end of the Hubble sequence. Color indicates there may be some recent, low star formation activity in the galaxy, but the overall characteristics point to a more quiescent and evolved system.
