The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge region that emits strongly in the observed bands, suggesting a high stellar density in the core. The color profile appears relatively uniform across the galaxy, with a subtle bluer tint extending outwards from the core, possibly indicating ongoing star formation or a younger stellar population in the outer regions. Overall, the galaxy displays a slightly elongated shape, with minimal evidence of spiral arms or significant disk structure. There appear to be no signs of active galactic nuclei activity or strong tidal disturbances in this image. The overall appearance is consistent with a relatively evolved galaxy undergoing passive evolution.
