This galaxy presents a generally smooth appearance with a central, bright bulge, suggesting an older stellar population concentrated in the core. The galaxy appears largely elliptical, exhibiting a moderate degree of roundness and a slight elongation. There is a subtle, extended halo surrounding the brighter central region. Some features are observable in the surrounding halo and galaxy itself, but its overall symmetry suggests a relatively relaxed system, without prominent signs of recent major merger activity. Faint blue tinges are evident within the central region and its disk, indicative of ongoing, albeit limited, star formation activity. The overall color suggests a mix of stellar populations. The size of the galaxy is roughly 5 kpc in radius.
