The galaxy presents as an elliptical morphology, exhibiting a smooth and diffuse light profile with no discernible spiral arm structures. The core is bright and concentrated, suggesting a high stellar density. The galaxy's overall shape is slightly elongated, indicating a moderate ellipticity. Color gradients are subtle, with a slightly redder hue towards the center and a bluer tinge in the outer regions, possibly indicating older stellar populations in the core and younger stars in the outskirts. There are no obvious signs of active galactic nuclei activity or significant dust lanes. The galaxy appears to be relatively undisturbed, without major tidal features or signs of recent mergers.