The galaxy presents a smooth, elliptical morphology. It appears to be primarily composed of older stellar populations, indicated by the redder, yellowish-orange hue dominating the central region. The light is concentrated towards the center, with a gradual decline in brightness towards the outer edges. No distinct spiral arms or bar structures are discernible. There's a subtle hint of bluer light at the fringes, suggesting the possibility of some ongoing star formation, albeit at a low rate. No significant signs of tidal disturbances, major mergers, or strong interactions with other galaxies are evident in this image. The galaxy is moderately luminous, and has a considerable mass. Its shape is closer to elliptical than disk-like.
