The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. The light distribution is concentrated towards the center, displaying a radial gradient with the core being the brightest and most intense. The overall shape is nearly circular, with only a slight suggestion of elongation. There's little evidence of spiral arms or significant dust lanes. The galaxy displays a reddish-yellow hue, indicative of an older stellar population with fewer young, massive stars and a cessation or slowing of star formation. Faint, diffuse emission extends outward from the central region, creating a halo-like appearance. There are no obvious signs of ongoing major mergers or significant tidal disturbances, though a minor asymmetry might suggest past interactions.
