The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and centrally concentrated morphology. It displays a bright, yellowish core, likely indicative of an older stellar population. The overall color gradient suggests a redder population in the central regions with bluer, younger stars potentially distributed sparsely throughout the outer edges of the galaxy. There is a faint, diffuse extension of light that could indicate a very small disk or tidal debris, but it seems more likely that is due to some other artifact. Based on the color and morphology, the galaxy is not particularly active in terms of star formation. The spheroidal shape and color profile align with characteristics expected for galaxies with a significant stellar mass. There is no evidence of active galactic nucleus activity or intense star formation regions.
