The galaxy presents as a somewhat smooth, elliptical-like structure, though with subtle features. There is a central concentration of light that diminishes gradually outwards, suggesting a relatively high degree of central mass concentration. The color appears to be slightly reddish/yellowish, suggesting an older stellar population, with a corresponding lower rate of star formation. There are no obvious spiral arms or bar structures visible. There may be some evidence of a minor disturbance, which could indicate a weak interaction with another galaxy, or a past minor merger event. Overall, this galaxy appears to be relatively isolated in its immediate environment.
