The galaxy presents as a disk-shaped system, oriented edge-on from our perspective. It exhibits a bright, concentrated central bulge or nucleus, indicative of a higher density of stars in that region. The disk component appears relatively smooth with some minor disturbances, lacking prominent, well-defined spiral arms. The overall color suggests a population of older stars, leaning toward redder wavelengths. The system's apparent ellipticity indicates a significant flattening of the disk. There might be a slight asymmetry or warp to the disk, possibly suggesting a previous minor interaction. The galaxy shows a consistent color profile. It has a moderate redshift which indicates that it is a relatively distant galaxy. The morphology suggests either an early-type spiral or lenticular galaxy, showing signs of a quiescent star formation rate.
