The galaxy presents as a somewhat amorphous structure, exhibiting characteristics of both a smooth elliptical galaxy and a possible disk galaxy. The central region displays a bright, concentrated luminosity indicative of a substantial stellar population. A fainter, bluer region extends from the main body, hinting at areas of more recent star formation. The overall shape is more elongated than circular, but not strongly barred or spiral in appearance. There are no clear signs of strong tidal disturbances or interactions with nearby galaxies, although there is a slight asymmetry that might suggest a minor disturbance. The galaxy's intermediate redshift suggests a considerable distance, which contributes to the blurring and smoothing of finer structural details.
