The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution suggests a high Sersic index, indicating a centrally concentrated profile. There is a slight elongation to the galaxy's morphology, and a subtle color gradient is observed from the core outwards, with the central region exhibiting a more yellowish hue, potentially indicating an older stellar population. Fainter, bluer regions are sparsely distributed in the outer areas of the galaxy, suggesting there may be small amounts of on-going star formation. No prominent spiral arms or distinct features are observed. The overall appearance indicates a galaxy that has undergone substantial evolution and may be nearing the end of its star-forming period.
