The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a generally rounded morphology with no obvious spiral arm structures or bar features visible in this image. There are no indications of a major ongoing merger, although minor tidal disturbances cannot be ruled out based on this image alone. The galaxy displays a significant red color, suggesting a population of older stars and a lower rate of star formation. The overall brightness profile suggests a concentration of stellar mass toward the center, typical of elliptical galaxies. Its moderate size indicates it is a galaxy of reasonable mass for its type.
