The galaxy appears as a somewhat elongated, elliptical structure, possibly indicative of an E4-E6 classification based on observed ellipticity. The central bulge exhibits a concentrated, bright yellow-orange hue, suggesting an older stellar population with a lower rate of star formation. Fainter, less-defined extensions are visible emanating from the core, hinting at a faint disk component, although the dominance of the bulge suggests it is a lenticular galaxy with a weak spiral arm structure or a bulge-dominated spiral galaxy. No significant dust lanes are visible, which is consistent with a passively evolving galaxy. There is no evidence of a recent major merger.
