The galaxy presents as an elliptical morphology, with a slight elongation. The luminosity profile appears relatively smooth and centrally concentrated, exhibiting a single nucleus. There is a change in the apparent color profile from the core outward. The galactic core shows a distinctive reddish hue, possibly indicating an older stellar population or significant dust obscuration. The outer regions exhibit a bluer color, which may suggest the presence of a younger, star-forming stellar population contributing to the light at bluer wavelengths. There is also a suggestion of some minor disturbance in the morphology, hinting at a possible interaction or merger event. Overall, the galaxy appears to be at an intermediate redshift, indicative of a relatively distant object.
