The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, tending towards roundness. The color profile appears to be dominated by older stellar populations, showing a strong yellow hue. The light is notably concentrated towards the core, with a gradual falloff in surface brightness towards the outer regions. There is little to no evidence of spiral arm structure or significant dust lanes visible in this image. Possible minor disturbance can not be ruled out, but based on the visual data presented, no major merger event is visible. 
