The galaxy appears to be a relatively smooth, elliptical system, exhibiting a centrally concentrated light profile. The core region is bright and yellowish in color, suggesting an older stellar population. There is evidence of what appears to be a secondary, smaller concentration of light situated near the main body, possibly indicating a minor interaction or merger event. The galaxy is not perfectly spherical, presenting a slight elongation. Overall, the galaxy does not show significant signs of recent or ongoing star formation and has the appearance of a evolved system with a substantial mass.
