The galaxy presents an elliptical morphology, exhibiting a smooth, featureless appearance with a high degree of central concentration. Its overall shape is elongated, with a major axis significantly longer than its minor axis. The light distribution is relatively uniform, lacking prominent spiral arms or distinct structural components. The galaxy displays a radial color gradient, with the central regions appearing more yellowish, gradually transitioning to a bluer hue in the outer regions, suggesting a potential gradient in stellar populations. This color profile hints at a population of older, redder stars concentrated in the galactic nucleus, with younger, bluer stars scattered in the outer regions. There are possible indications of minor disturbances in the outer halo region.
