The galaxy presents as a primarily smooth, elliptical structure. The central region displays a bright, concentrated luminosity, suggesting a dense nucleus likely composed of older stellar populations. Moving outwards from the core, the light intensity gradually diminishes, forming a more diffuse halo.

While the overall structure is smooth, there appears to be some subtle irregularity in the outer regions, hinting at possible minor disturbances. The galaxy’s color profile suggests a redder overall hue, further supporting the presence of an older stellar population. The galaxy lacks any obvious spiral arm structures, nor does it exhibit a prominent disk feature. There is no conclusive evidence of a major ongoing merger, but the subtle distortions may indicate a past interaction.
