The galaxy presents an elliptical morphology, exhibiting a smooth, centralized luminosity profile. A bright, yellowish core dominates the galactic center, suggesting a high concentration of older stellar populations. The galaxy's outer regions display a gradual decrease in brightness, fading into a less defined halo. A subtle, bluish tint is observed in some regions, possibly indicating areas of more recent star formation, although this is not the primary characteristic. There is no prominent disk structure or spiral arm morphology visible; the light distribution is largely symmetric around the central core. No significant signs of tidal disruption or ongoing mergers are clearly evident in this imagery.