The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a predominantly round shape with a noticeable lack of spiral arm structures or a distinct disk component. The color profile shows a gradient, trending towards redder hues in the central regions. The galaxy appears relatively undisturbed, showing no signs of major merging events or tidal distortions. The object's overall light distribution suggests an evolved stellar population. The galaxy appears moderately bright, with an estimated effective radius of roughly 5 kiloparsecs, suggesting a galaxy of significant size. Star formation appears suppressed overall, as the galaxy's color implies a diminished quantity of young, massive stars.
