The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile. The central region exhibits a yellowish-orange hue, suggesting a population of older stars. Moving outward from the core, there is a slight color gradient towards a bluer tinge, hinting at the presence of a younger stellar population, or possibly low level star forming regions on the periphery. No distinct spiral arm structure or prominent dust lanes are discernible. The shape is moderately elongated, closer to round, but showing a definite elliptical form. There are no signs of tidal disturbances or ongoing merger activity in the image. The galaxy appears relatively isolated and undisturbed. Overall, it is consistent with a relatively massive galaxy with a moderate redshift, a considerable mass, and a likely subdued star formation rate.
