The galaxy appears as an elongated, elliptical structure, exhibiting a smooth morphology. The central region is characterized by a bright, concentrated core, with the light intensity gradually decreasing towards the outer edges. The color profile suggests a generally older stellar population, displaying a yellowish-red hue indicative of evolved stars. There is a subtle hint of a disk-like structure, but it is not well-defined. No prominent spiral arms or dust lanes are discernible. Overall, the galaxy presents an appearance consistent with a mature system, with minimal signs of ongoing star formation activity.
