The galaxy presents as a relatively smooth, centralized object, appearing elliptical in shape. The light profile indicates a concentrated central bulge with a gradual decrease in luminosity outwards. There is a subtle color gradient, with the core appearing slightly more yellow or orange, suggesting an older stellar population. The outer regions show hints of blue, which could be indicative of younger stars, but this is marginal. There is no prominent disk structure, spiral arms, or any signs of strong tidal interactions or major merging events visible. There may be some minor disturbance or faint features in the outskirts of the halo, but the image resolution limits any definitive assessment. Overall, it appears as a fairly regular and well-formed elliptical galaxy at a moderate redshift.
