The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a yellowish-orange hue, suggesting an older stellar population. There is no clear evidence of spiral arm structures or significant dust lanes. The galaxy's shape is generally elliptical but also rounded, with a slight deviation from perfect circularity. Faint, diffuse extensions are tentatively visible in the surrounding halo, indicating a possible interaction or recent merger event. The core region appears to have a higher concentration of stellar density, and the halo gradually fades away.