The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The color profile suggests a population of older stars dominating the light output, indicated by the yellowish-red hue. There is no apparent spiral arm structure or significant dust lane features visible in the image. The galaxy appears to be fairly isolated and undisturbed. The round morphology suggests it has likely undergone significant evolution. It appears to be a fairly massive galaxy with a low star formation rate.
