The galaxy presents as a relatively smooth, elliptical structure, with a high degree of central concentration. The light profile appears to gradually decrease from the bright, yellowish core outwards. There is no discernible spiral arm structure or prominent dust lane. The galaxy's overall color appears to be trending towards redder wavelengths. The morphology suggests a galaxy that is largely devoid of active star formation, possibly indicative of an older stellar population. Subtle disturbances or asymmetries are not obviously apparent. It appears largely isolated, with no immediately interacting companions. The overall form suggests a relaxed, evolved system.
