The galaxy presents as a moderately luminous object, displaying a smooth, elliptical morphology with a slightly elongated profile. The central region exhibits a concentrated, bright core, indicative of a possible bulge component. There is a noticeable color gradient, shifting from a yellower, warmer hue in the core to a bluer, cooler tone in the outer regions. No prominent spiral arms or distinct features are discernible, suggesting a relatively passive system. The overall appearance indicates a galaxy with a likely low star formation rate and a dominant population of older stars.
