The galaxy presents as a centrally concentrated, elliptical-like structure. There is an apparent lack of distinct spiral arms or a well-defined disk. The light profile appears relatively smooth with a fairly regular morphology. There's a subtle color gradient observed, transitioning from a slightly bluer hue in the core region to subtly redder tones in the outer regions. This could indicate a varying stellar population, with younger stars potentially concentrated towards the center. There is no indication of a major merger or significant tidal disturbances. The galaxy appears fairly isolated and undisturbed within its immediate environment.
