The galaxy presents a generally smooth and elliptical morphology, with a concentrated central bulge. There appears to be some evidence of a surrounding disk component, although the disk is faint and not sharply defined. Color gradients suggest that the central region is dominated by older stellar populations, exhibiting a yellow-orange hue. Moving outward from the center, the color shifts slightly toward bluer tones, possibly indicating regions of more recent star formation, albeit at a modest rate. There are no indications of strong tidal features, major mergers, or significant disturbances. The overall structure is relatively symmetrical and well-defined. The system is likely a massive galaxy with a moderate rate of star formation.
