This galaxy presents as a relatively smooth, elliptical structure, with a concentration of light towards its central region, indicative of a galactic nucleus. There is a noticeable color gradient, shifting from yellow/orange hues in the core to slightly bluer tones in the outer regions. The light distribution is relatively uniform, with no distinct spiral arm structures apparent. The galaxy exhibits a moderate degree of ellipticity, appearing more rounded than elongated. There are no obvious signs of ongoing mergers or major disturbances, though subtle irregularities in the outer regions cannot be entirely ruled out based on this image alone. The galaxy appears to be a fairly mature system, dominated by older stellar populations, although the presence of bluer color in the outer regions may suggest some recent, albeit subdued, star formation activity.
