The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. Its color gradient indicates a stellar population that is predominantly older, resulting in a yellowish-orange hue. There appears to be minimal evidence of recent star formation. The overall structure suggests a system that has largely completed its period of major mergers, with no significant tidal features or strong morphological disturbances visible. The galaxy appears to be relatively isolated. The isophotes appear regular and undisturbed, consistent with a relaxed, dynamically evolved system.
