The galaxy presents as a single, concentrated body with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. There is minimal evidence of spiral arm structures or significant dust lanes. The outer regions of the galaxy fade gradually into the background sky, indicating a lack of sharp edges or distinct features. Overall, the galaxy appears to be a relatively undisturbed, well-formed elliptical galaxy with high central density.
