The galaxy presents as a slightly elongated, smooth object. The central region exhibits a brighter, more concentrated luminosity, indicative of a core. Moving outward from the center, the light gradually diffuses, transitioning into a fainter, extended halo. The overall color appears to be consistent, suggesting an older stellar population with minimal active star formation. There is a subtle hint of asymmetry in the halo's extension, with one side appearing slightly more elongated. No distinct spiral arms or dust lanes are discernible. Based on the overall morphology, this galaxy appears to be an elliptical galaxy, or possibly a lenticular galaxy viewed from a great distance. There is no significant evidence of recent mergers or major disturbances in its structure.
