This galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, indicating a central bulge likely composed of older stellar populations. The galaxy appears largely spheroidal, exhibiting high degree of roundness, with only a slight departure from a perfectly circular shape. There's a noticeable lack of distinct spiral arms or other prominent features, suggesting a relatively quiescent or post-star-forming stage. The galaxy's color suggests a moderate redshift. The smooth light distribution and lack of strong color gradients point towards a relatively homogeneous stellar population. The galaxy does not show any obvious signs of ongoing major merger activity.
