The galaxy presents a largely elliptical morphology, exhibiting a smooth, featureless light distribution. The central region is characterized by a high surface brightness core, appearing yellowish in color, suggesting a concentration of older stellar populations. A faint, extended halo surrounds the core, with colors transitioning to redder hues further from the center. No distinct spiral arms or dust lanes are discernible. The overall structure indicates a relaxed, dynamically evolved system with minimal recent star formation activity. There is no apparent evidence of tidal disturbances or ongoing mergers, suggesting a relatively isolated existence. The galaxy exhibits a slightly elongated shape, but lacks significant asymmetry.
