The object appears to be a galaxy exhibiting characteristics of a merger event. There is a prominent, roughly spherical central component, with a smooth appearance and yellowish hue, which is characteristic of older stellar populations. Located to the right of the main component, there is a smaller, less defined object. There are no clear spiral arm structures visible. The overall morphology suggests a system undergoing interaction, which might result in a future elliptical galaxy, or potentially a disturbed disk galaxy. The relatively uniform color suggests a low ongoing star formation rate, with a higher concentration of older stars.
