The galaxy presents a primarily smooth morphology, appearing largely elliptical in shape. The core region displays a bright, somewhat irregular structure with a hint of blue coloration. This possibly indicates recent or ongoing star formation activity, although it could be artifacts from the imaging process. Extending outwards, the galaxy exhibits a more diffuse, yellowish halo, suggestive of an older stellar population. There is a subtle indication of a faint disk, but any spiral arm structure is not clearly visible. The galaxy seems relatively isolated, with no obvious signs of major tidal disturbances or mergers in the immediate vicinity.
