The galaxy presents a generally smooth, elliptical morphology. The core exhibits a concentrated, bright yellowish-white luminosity. A faint, more diffuse halo surrounds the core, extending outward with a slightly elongated shape. The color gradient suggests older stellar populations dominate the galaxy. No distinct spiral arms or dust lanes are discernible. There is a suggestion of possible gravitational disturbance within the structure of the galaxy itself, but further investigation would be needed to confirm a merger or tidal interaction.
