The galaxy presents a generally smooth and rounded morphology, exhibiting a high degree of central concentration with a bright core. The light distribution appears relatively uniform, indicative of minimal resolved substructure. Faint, diffuse extensions are observed, surrounding a bright, yellowish central region. There is a slight color gradient, transitioning from a yellowish hue in the center to a bluer tint toward the outer regions, which may suggest a difference in stellar populations. No distinct spiral arms or prominent dust lanes are discernible in this image. The shape appears largely elliptical or spheroidal. There is no obvious indication of a major ongoing merger event, although minor asymmetries cannot be entirely ruled out.
