The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. Color gradients are subtle, with the core region exhibiting a yellowish hue, suggesting an older stellar population. The outer regions appear slightly bluer, potentially indicating the presence of younger stars, though the overall blue light contribution is minimal. There is a slight elongation, giving the galaxy a cigar shape. No obvious spiral arms or dust lanes are apparent. The galaxy appears relatively undisturbed, with no strong visual evidence of recent or ongoing major mergers, although there is the possibility of minor disturbances present. Based on color and morphology, this galaxy appears to be a relatively massive system.
