The galaxy presents a somewhat elliptical morphology, appearing mostly smooth in structure. A concentrated, yellowish central bulge dominates the galaxy's core, which has a fairly high degree of roundness. Surrounding the bulge is a fainter, bluer disk, suggesting regions of recent star formation. There is a faint asymmetry, suggesting a minor disturbance, such as a past merger event or tidal interaction, although no prominent tidal tails or obvious merger remnants are visible. Overall, the galaxy appears to be relatively undisturbed and displays characteristics of a typical disk galaxy at a moderate redshift, with an estimated size of approximately 6 kpc. The color indices indicate that the galaxy is composed of an older stellar population in the bulge and younger stars in the disk.
