The galaxy presents as a relatively smooth, centrally concentrated object. The core region exhibits a bright, yellowish-white luminosity, suggesting an older stellar population and/or significant dust obscuration. This bright central region appears to fade gradually outward. The overall shape of the galaxy is somewhat elliptical with an axis ratio that suggests it is close to face on. There is no immediately obvious evidence of significant spiral arm structure, or other features usually associated with galactic disks. No strong signs of recent or ongoing major merger activity are apparent upon visual inspection. Faint irregular features could possibly indicate minor disturbances in the outer regions. The color profile of the galaxy suggests a relatively homogenous stellar population across the observable region.
