The galaxy presents as an elongated, spindle-shaped structure. The light distribution suggests a central bulge that is brighter and more diffuse than the rest of the galaxy. The overall color profile is indicative of an older stellar population, with redder hues dominating. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. There is a hint of a fainter, bluer region, potentially indicating some ongoing, albeit low, star formation activity. The morphology is most consistent with that of an elliptical galaxy.
