The galaxy appears to be a relatively compact, well-defined elliptical galaxy. Its morphology suggests a smooth, spheroidal structure with a high degree of circular symmetry. There's a hint of a faint disk-like structure, possibly an indication of an inner disk component viewed close to edge-on, but the overall light distribution is dominated by a smooth, centrally concentrated bulge. The color profile indicates a redder overall population suggesting older stellar populations dominating, with a lack of substantial ongoing star formation. No prominent dust lanes or tidal features are immediately visible. There may be a slight asymmetry along the major axis, but further data is needed to confirm if that indicates a possible interaction or minor merger event in the past.
