The galaxy presents as a generally smooth, elliptical morphology. Its light profile appears concentrated towards the center, with a gradual decrease in intensity outwards. The core region exhibits a yellowish hue, potentially indicating an older stellar population. Progressing outwards, the galactic disc becomes more bluish, maybe a sign of recent star formation. The axial ratio indicates the galaxy is elongated with the major axis running horizontally. There is no apparent bar structure, spiral arm morphology, or significant dust lane obscuration. The overall appearance suggests a mature system with a low star formation rate. No merger activity or tidal features are discernible.