The galaxy presents as a somewhat smooth, centrally concentrated object with a general elliptical morphology. There are no clear spiral arm structures or a prominent disk component visible in this image. The galaxy exhibits a relatively uniform color profile, with a slight color gradient that indicates older stellar populations dominate, consistent with that of an elliptical galaxy at a moderate distance. There appears to be a slight flattening, suggestive of a deviation from a perfect sphere. There are no apparent signs of major mergers or significant tidal disturbances; however, faint, subtle features possibly indicate minor interactions or internal dynamical processes. The overall appearance points towards a galaxy that has largely exhausted its star-forming material, although a small amount of ongoing star formation is still present.
