The galaxy presents as a relatively smooth, centralized object. It exhibits a generally elliptical morphology with a high degree of radial symmetry. The galaxy possesses a bright central core, suggesting a concentration of stellar density or perhaps an active galactic nucleus, though the resolution limits definitive confirmation. The color profile transitions from a yellow-white core to a bluer outer halo. This color gradient could imply varying stellar populations, with older, redder stars concentrated centrally and younger, bluer stars residing in the outer regions. There is a very slight asymmetry in the outermost regions, though there does not appear to be a major disturbance, merger, or tidal tail present. The galaxy's overall appearance is consistent with that of a relatively massive early-type galaxy, likely at an intermediate redshift.
