This galaxy presents as a relatively smooth, elliptical structure with a moderately elongated shape. The central region displays a higher concentration of light, suggesting a prominent galactic nucleus. The overall color appears to be on the redder side, indicative of an older stellar population with limited ongoing star formation. Faint, diffuse light extends outwards from the central region, forming a less distinct halo. There is little evidence of spiral arm structures or significant dust lanes. Close inspection does not reveal signs of major disturbances that would suggest recent or ongoing merger activity, though minor tidal features might be present. Overall, this galaxy exhibits characteristics consistent with an elliptical galaxy at an intermediate redshift, likely composed of primarily older stars with a relatively low rate of current star formation.
