The galaxy presents as a relatively smooth, elliptical object. Its overall color profile suggests a dominant population of older stars, exhibiting a yellowish hue in the central region. The light becomes slightly bluer moving towards the periphery, potentially indicating some degree of recent or ongoing star formation in the outer regions, albeit at a low level. The galaxy appears somewhat elongated but not highly so. There is no clear evidence of spiral arms or a distinct disk structure. The central bulge is prominent and appears to be the brightest region. No obvious signs of major mergers or tidal disturbances are visible, suggesting a relatively quiescent evolutionary history.
