The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, appearing yellow-white in color, suggesting an older stellar population. Fainter, more diffuse light extends outwards from the core, transitioning to a redder hue, which may indicate the presence of some ongoing, albeit moderate, star formation in the outer regions. No spiral arm structure is discernible. There is very little dust or gas visible. The overall appearance suggests this is a relatively mature galaxy. There are no obvious signs of a major ongoing merger or significant tidal disturbances.
