The galaxy presents a largely smooth, elliptical morphology. The central bulge exhibits a yellowish-white hue, possibly indicating an older stellar population. A faint disk structure is observable, exhibiting bluer tones. This hints at the presence of ongoing star formation. The overall shape appears largely round, with minimal signs of significant tidal disturbances or interaction with neighboring galaxies, though subtle asymmetries cannot be ruled out. The galaxy's integrated light suggests a moderately massive system with a corresponding rate of star formation.
