The galaxy presents as an elliptical morphology with a smooth, diffuse light distribution. The color gradient suggests a relatively evolved stellar population, with a central concentration of older, redder stars. A subtle disk-like structure is possibly present, with a minor bluer component indicating ongoing, but low-level, star formation. There is no obvious indication of strong tidal features or interactions with other galaxies. The galaxy appears to be a relatively isolated system exhibiting a moderate redshift. It has a central bulge with a fairly low surface brightness.
