The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a bright, yellowish-orange hue, indicative of an older stellar population. Surrounding this core is a fainter, more diffuse halo exhibiting bluer tones. The halo appears relatively smooth. There are no apparent spiral arm structures or significant dust lanes visible, and no apparent signs of active galactic nuclei activity. There may be a minor gravitational disturbance. Overall, the galaxy appears to be an evolved system, likely undergoing relatively low levels of star formation. Its estimated physical size is roughly 7 kpc in radius, and it is relatively massive. The estimated redshift of approximately 0.25 indicates that we are observing this galaxy as it was several billion years ago.
