The galaxy presents as a largely featureless, elliptical morphology. It exhibits a concentrated central bulge that transitions smoothly outward into a less dense halo. The core appears yellowish-white, suggesting a population of older stars. The outer regions of the galaxy fade into a diffuse blueish haze, perhaps indicating more recent, albeit limited, star formation. There is no strong evidence of spiral arms or significant dust lanes within the observed wavelengths. It seems to be an isolated galaxy with no apparent signs of recent merger activity or significant tidal disturbances. Overall, the galaxy seems to be an evolved system.
