The galaxy presents as an elliptical morphology, appearing mostly smooth with a high degree of central concentration. The light profile is dominated by a bright, yellowish core, suggestive of an older stellar population or dust extinction. The isophotes are largely regular and elliptical, with only a slight deviation from perfect roundness. There is no apparent disk structure, spiral arms, or bar. Faint, diffuse extensions of light can be observed surrounding the main body, hinting at a substantial halo component or possible tidal interactions, though no clear signs of ongoing major mergers or significant disturbances are visible. The color gradient suggests a potential redshifting of light from core to edge indicating, perhaps, an older stellar population in the outer regions.
