The galaxy presents as a mildly elliptical structure with a smooth, relatively featureless morphology. The central region exhibits a bright, concentrated core, indicative of a substantial stellar population and possibly an active galactic nucleus. The overall color profile suggests a generally older stellar population, with a noticeable lack of prominent blue regions that would signify ongoing, significant star formation. Faint, diffuse extensions are potentially observable, though these are not well defined, giving the galaxy a fuzzy appearance at its edges. There is no strong evidence of spiral arms or a well-defined disk. The morphology suggests it could be an elliptical galaxy, but the intermediate "roundness" and "in-between" characteristics point to it possibly being somewhere between an elliptical and a lenticular galaxy type. Minor disturbances can not be ruled out, even though the main body looks pretty much undisturbed.
