The galaxy presents as a largely featureless, smooth object, exhibiting a generally elliptical morphology. Its color profile leans towards the red end of the spectrum. There is little to no visual evidence of spiral arm structure or prominent dust lanes. The overall roundness is quite high, with no significant elongation or distortions suggesting major ongoing mergers, although minor disturbances cannot be ruled out. There appears to be a high degree of symmetry about the center, suggesting that it has likely reached a dynamically relaxed state. Any on-going star formation is estimated to be low.
