The galaxy presents as a centrally concentrated, smooth, elliptical-like structure. There is a clear radial gradient in luminosity, with a bright, nearly unresolved core. The color is generally yellowish-red, indicating an older stellar population. There may be a faint disk with subtle disturbances. The smooth morphology suggests the possibility of a prior merger event, and a general lack of significant ongoing star formation. The galaxy does not show a distinct spiral arm structure or any prominent dust lanes. The galaxy appears relatively isolated and not obviously interacting with any companion galaxies.
