The galaxy presents a generally smooth morphology, with a high degree of central concentration, and a slight amount of asymmetry. Its shape appears to be generally disk-like, but is overall relatively smooth. The core exhibits a bright yellow-white hue, suggesting a concentration of older stellar populations. There is a gradual decline in luminosity moving outward from the core, with the galaxy's color shifting towards a more reddish hue in its outer regions. This may indicate some ongoing or recent minor star formation within the disk, but at a relatively low rate. There is no indication of significant tidal disturbances or ongoing mergers. The galaxy's appearance suggests a relatively evolved system, possibly a spiral galaxy with a dominant bulge and a relatively weak disk, or an elliptical galaxy. Its intermediate redshift places it at a significant cosmological distance, making detailed structural analysis challenging.
