The galaxy presents an overall smooth morphology, with a somewhat elliptical shape. The central region exhibits a bright, concentrated luminosity, likely indicative of a significant stellar population or active galactic nucleus. A faint, extended disk-like structure surrounds the central bulge. There is a slight color gradient visible, with the central region appearing more yellow-white, possibly indicating older stellar populations, while the outer regions display a hint of bluer light, suggesting the presence of younger stars or ongoing star formation. There is a subtle asymmetry in the outer regions, but no prominent features suggestive of major disturbances or ongoing mergers are immediately apparent.
