The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth light distribution. There's a noticeable color gradient, transitioning from a redder core to bluer outer regions. This could indicate older stellar populations concentrated toward the center and younger stars in the surrounding areas. The overall morphology lacks prominent spiral arms or distinct features, suggesting a more evolved system. The relatively smooth profile and lack of significant disturbances do not strongly suggest an ongoing major merger event, though subtle irregularities may indicate minor interactions. The galaxy appears to be moderately luminous.
