This galaxy presents a relatively smooth and rounded morphology. It exhibits a bright, concentrated central bulge which gradually diffuses into a fainter, more extended halo. There is some subtle bluing along the outer edges of the galaxy, indicating ongoing, but perhaps subdued, star formation activity. No distinct spiral arm structures are visible, and the overall appearance suggests an elliptical or lenticular type galaxy, with no major mergers or disturbances. The galaxy appears fairly isolated in this field, with no obvious tidal features or interactions affecting its morphology.
