The galaxy presents as a relatively bright, elliptical object with a significant central bulge. The core exhibits a yellow-orange hue, suggesting an older stellar population. Fainter, bluer regions are present at the periphery, possibly indicating areas of more recent star formation, especially on the left side. There are faint indications of disturbed morphology, with the possibility of tidal tails. The presence of these tails suggests a possible interaction or merger event in its past, as well as some merger activity currently. The smooth and symmetrical light profile of the galaxy, coupled with the color gradient from the core outwards, is consistent with an evolved galaxy with a substantial mass. 
