The galaxy presents as an elliptical morphology, with a relatively smooth light distribution. The core exhibits a bright, concentrated yellowish hue, suggesting an older stellar population. This central region is surrounded by a less luminous, more diffuse halo with a slight bluish tint. The overall shape is nearly circular. There is no visible evidence of spiral arms or significant dust lanes. There appears to be a very slight disturbance to the overall smoothness of the galaxy, though there is no significant sign of a merger.
