The galaxy appears to be an elliptical galaxy, exhibiting a smooth, nearly spherical morphology. The light distribution is highly concentrated toward the center, with a bright, yellowish core indicative of an older stellar population. There is a gradual decrease in luminosity from the core outwards, without any apparent spiral arm structures or dust lanes. The overall color suggests a lack of significant ongoing star formation, dominated by evolved, redder stars. Subtle color gradients might be present, but the limited resolution hinders detailed analysis of these features. There are no signs of tidal disturbances or ongoing mergers that would be visible at this resolution, although minor interactions cannot be ruled out.
