The galaxy appears to be an elliptical galaxy with a smooth, concentrated light profile. It exhibits a generally round morphology, although a slight elongation along one axis is observable. The core is bright and dominates the overall luminosity of the galaxy. The light appears to be a yellow/white color. There are no clearly defined spiral arms or dust lanes visible, suggesting a lack of significant ongoing star formation. There is a slight asymmetry in the light distribution, with a subtle extension or faint halo present on one side, which may indicate a past minor merger event or tidal interaction. The central region is consistent with an older stellar population, which could potentially be a supermassive black hole at the center. There are no obvious signs of strong tidal features or a major ongoing merger.
