The galaxy presents an elliptical morphology, with a smooth, centrally concentrated bulge dominating the overall structure. There is a subtle disk-like structure, however no clear spiral arm features are observed. The color gradient suggests a significant population of older stars within the bulge, exhibiting a reddish hue, with hints of more recent star formation in the outer regions, showing bluer colors. The galaxy appears undisturbed, with no obvious signs of recent merger activity or tidal distortions. It appears to be a relatively massive galaxy with a moderate rate of star formation.
