The galaxy presents as a predominantly smooth, elliptical structure. The core is a bright, concentrated yellow-white, suggesting a high density of older stellar populations. There is a slight elongation of the galaxy, but it maintains a generally rounded shape. A faint, diffuse halo extends outwards from the central bulge, gradually fading into the background. No distinct spiral arms or significant dust lanes are discernible in this image, implying a relatively undisturbed morphology. There is no visual evidence of any major ongoing merger activity. The galaxy's color indicates a general lack of current high star formation activity.
