The galaxy appears to be a relatively smooth and concentrated elliptical galaxy, likely at an intermediate redshift. It presents with a near-spherical morphology, showing little to no evidence of a disk-like structure. There is a bright, centrally located bulge that dominates the galaxy's overall luminosity. The color profile suggests an older stellar population, indicated by a redder hue, possibly indicating a lower rate of on-going star formation. A subtle extension of light around the central region may indicate a diffuse halo or the presence of a weak stellar stream. The smoothness of the galaxy implies it may have undergone a major merger event in the past. The lack of clear tidal features suggests that any recent interactions were minor or occurred in the distant past.
