The galaxy appears to be a lenticular or early-type spiral galaxy, displaying a predominantly smooth and featureless morphology. The central bulge is prominent and gradually fades into a surrounding disk. The galaxy's overall shape tends towards an elliptical form rather than a clearly defined spiral structure, lacking prominent spiral arms or distinct dust lanes. There is a subtle color gradient, with the core appearing brighter and slightly yellow-white in color, suggesting an older stellar population. The outer regions show a faint bluish tinge, possibly indicating the presence of a small population of younger, hotter stars. No signs of major mergers are visible, though subtle distortions might suggest minor past interactions. The low star formation rate also indicates that this galaxy is likely near the end of its life cycle. The galaxy is relatively compact.
