The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears centrally peaked, with a gradual falloff in intensity towards the outer regions. The dominant color is a yellow-orange hue, suggesting an older stellar population with lower levels of ongoing star formation. The galaxy exhibits a generally round morphology, with no obvious signs of a disk component or spiral arms. There is a subtle color gradient, with the central regions appearing slightly redder than the surrounding areas, indicative of possible age or metallicity differences within the galaxy. No major signs of tidal disturbances or recent merger events are immediately apparent in the image, though subtle asymmetries could be present upon closer inspection. Overall, the galaxy appears to be a relatively evolved system, with a significant fraction of its stellar mass already in place.
