The galaxy presents as an elliptical morphology, displaying a relatively smooth, symmetrical light distribution with no prominent spiral arms or bar structure visible in this image. It exhibits a somewhat rounded appearance. The central region is brighter and more concentrated, gradually fading towards the outer edges. Color analysis indicates the galaxy is dominated by older stellar populations which emit in the redder wavelengths. There is no indication of significant recent star formation within the galaxy based on the color. The image suggests the galaxy does not show strong evidence of ongoing mergers or tidal disturbances. The object appears as a relatively isolated system with no nearby companion galaxies causing significant gravitational interactions. The galaxy has an apparent size, as shown in the image, that suggests its a considerable physical size at its given distance.
