The galaxy presents a relatively smooth, elliptical morphology. The light distribution suggests a central concentration, with a gradual decrease in surface brightness outwards. The core region exhibits a yellowish hue, possibly indicating an older stellar population. Fainter, bluer light surrounds the yellowish core, which may indicate some ongoing, though limited, star formation. There is no clear evidence of spiral arms or a distinct disk structure, and the galaxy appears largely undisturbed, showing no significant signs of mergers or tidal interactions. The overall appearance points towards a galaxy that is moderately massive.
