The galaxy presents as a somewhat elliptical, relatively smooth structure. The central region exhibits a concentrated, bright core, indicative of a significant stellar population and/or active galactic nucleus. The galaxy displays a yellowish-red hue, suggesting a population of older stars and possibly dust obscuration. There may be a hint of faint, extended structure or a very diffuse disk, but overall the galaxy appears fairly featureless. No strong indications of spiral arms or significant star-forming regions are visually apparent in this image. Minor disturbances or signs of merging are not obviously detected. The galaxy appears to be a relatively undisturbed system.
