The galaxy presents a primarily smooth, elliptical morphology. It exhibits a relatively concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The shape is moderately rounded, with a slight deviation from perfect circularity, suggesting a possible minor interaction or internal asymmetry. No significant dust lanes or spiral arm structures are visible. The color is generally consistent across the galaxy, with a subtle trend towards redder hues in the central regions and slightly bluer tinges towards the outer edges. This color gradient may indicate a central population of older stars and a younger stellar population in the periphery. There is no apparent evidence of ongoing major mergers or tidal disturbances. The overall structure suggests a galaxy in a relatively late stage of evolution, possibly transitioning towards a more passive state of star formation.
