The galaxy appears to be a relatively smooth elliptical galaxy. It exhibits a concentrated, circular morphology, with a high degree of central bulge dominance. There is little evidence of spiral arms or a prominent disk. The light distribution suggests an older stellar population, with a yellowish-orange hue dominating the galactic core, possibly indicating lower levels of recent star formation. No significant tidal features or signs of ongoing mergers are clearly visible. The galaxy appears relatively isolated and unperturbed.
