The galaxy presents as a disk-shaped system, observed at a relatively high inclination. A prominent bulge region is visible at the galaxy's center, appearing concentrated and exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk component displays bluer tones and is relatively smooth. The dust lanes within the disk are not obviously detectable, however there are hints that the disk is not perfectly smooth and shows some signs of a spiral structure. The system does not obviously show any signs of any major merger events, or significant tidal disturbances in its morphology. The overall color suggests an intermediate redshift galaxy.
