The galaxy presents as a roughly elliptical, somewhat irregular structure. The core exhibits a high degree of central concentration, appearing smooth and luminous with a yellowish hue indicative of an older stellar population. A faint, diffuse halo surrounds the core, extending further along what appears to be the major axis. The halo exhibits subtle colour variations, transitioning from a yellow-white close to the core to a slightly bluer tinge at the periphery. This may indicate younger stars or ongoing star formation. There's a hint of asymmetry in the outer regions, suggesting possible minor disturbances, perhaps from a past interaction or minor merger event. No distinct spiral arm structure or dust lanes are visible. The overall appearance points towards a relatively evolved system.
