The galaxy appears as a relatively smooth, elliptical-like object with a high degree of central concentration. The light profile transitions gradually from a bright, yellowish core to a more diffuse halo. There is a possible secondary, smaller condensation of light near the main body of the galaxy which could possibly indicate a companion or tidal feature. No obvious spiral arm structures or dust lanes are discernible. The overall color suggests an older stellar population. The galaxy shows no strong signs of ongoing major mergers or significant tidal disruptions, although a minor interaction cannot be ruled out. The morphology appears to be generally undisturbed.
