The galaxy presents as a relatively smooth, elliptical form. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The core region exhibits a slightly yellowish-orange hue. There are no apparent spiral arm structures or prominent dust lanes visible within the resolution of this image. The galaxy appears fairly isolated, with no immediate signs of ongoing major merger events. There may be some evidence of minor disturbances in its morphology, though these are not definitively confirmed by this image.
