The galaxy presents as an elliptical morphology, with a smooth, diffuse light profile and high degree of central concentration. There is no apparent disk structure or spiral arm formation. The galaxy appears to be generally spheroidal with a slight elongation. The color gradient indicates a population of older stars, though some blue emission indicates regions of moderate star formation. There is no sign of an ongoing major merger or significant tidal disturbances, though the presence of minor disturbances cannot be ruled out based on the image alone.
