The galaxy appears to be a slightly elongated, early-type system at a moderate redshift. It exhibits a generally smooth morphology, with a centrally concentrated luminosity profile. The core of the galaxy is noticeably brighter and displays a yellowish hue, suggestive of an older stellar population. Fainter, bluer regions of star formation may be present, but are not dominant in the overall color profile. There are no obvious signs of a major ongoing merger, though subtle disturbances cannot be ruled out. The overall structure is moderately rounded, lacking the clear disk-like features of spiral galaxies.
