The galaxy presents a generally smooth morphology. The central region exhibits a concentrated luminosity, appearing yellowish-white, indicative of a potentially older stellar population. Extending outwards from the center, the light gradually diminishes, transitioning into a more reddish hue, hinting at either a fading stellar population or increased dust obscuration. A subtle extension can be seen in the top left of the galaxy that is more blue in color, indicative of some star formation. The overall shape appears elongated, not perfectly spherical, showing an elliptical structure. There are no prominent spiral arms or distinct features readily apparent in the image, suggesting it is likely an early-type galaxy, possibly an elliptical or lenticular galaxy viewed at an angle. There is no obvious indication of a major merger event, but some minor interaction cannot be ruled out based on the smoothness.
