The galaxy presents as a relatively compact, elliptical-like structure with a smooth appearance, indicating a lack of prominent spiral arms or complex features. It displays a somewhat spherical morphology, exhibiting a high degree of roundness. Its light is predominantly distributed uniformly, with a concentration of intensity in the center, suggesting a higher density of stars or active galactic nucleus (AGN) activity, though the resolution makes it difficult to confirm. Color gradients seem subtle, possibly indicating an older stellar population. The galaxy appears isolated with no obvious signs of ongoing major merger activity or strong tidal disturbances. Minor irregularities in shape or luminosity are challenging to assess due to image resolution, but the general absence of strong distortions implies stability in its structure. The galaxy's light is notably redshifted.
