The galaxy appears as an elliptical structure, exhibiting a smooth and featureless morphology. The light distribution suggests a centrally concentrated spheroid with a gradual decrease in luminosity towards the outer regions. There is no apparent spiral arm structure or dust lane obscuration visible in this image. The galaxy exhibits a slight elongation along one axis, but maintains an overall rounded appearance. The color profile indicates a relatively evolved stellar population, with a yellowish-white core grading into a slightly bluer halo. This color gradient may suggest ongoing, but low levels of star formation in the outer regions of the galaxy, or a population of younger stars within the halo. There is no evidence of any major interaction or merger events, although subtle asymmetries could be present, warranting further investigation.
