The galaxy presents as a predominantly smooth, elliptical-like structure. It exhibits a high degree of central concentration with a bright core. The radial light profile appears to decline smoothly from the core outwards. There is a faint, diffuse extension or plume visible at the top. This galaxy has a slight color gradient, appearing bluer toward the outer regions and redder towards the center. The shape is largely round, showing minimal deviation from circular symmetry. There is no distinct evidence of a prominent disk structure, spiral arms, or significant ongoing merger activity, although the top plume may indicate a previous interaction.
