The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. A bright, prominent core dominates the galaxy's structure, indicating a likely massive stellar population and/or an active galactic nucleus. The color appears generally red-shifted, particularly towards the galactic center, suggesting an older stellar population with limited ongoing star formation. The outer regions display a fainter, diffuse glow, gradually fading into the background. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There might be subtle hints of a very faint disk structure, but further, higher resolution data is required.
