The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of central concentration. Its overall shape is nearly circular. The color profile indicates a generally older stellar population, as suggested by the redder hue concentrated in the core. A subtle greenish tint, likely due to some star formation activity, is faintly visible in its body. No prominent spiral arms, bar structure, or signs of major interaction or ongoing merger events are discernible. It is characterized by moderate luminosity.
