The galaxy presents a dual morphology, exhibiting both a smooth, concentrated component and a fainter, more diffuse structure.

One component is characterized by a centrally concentrated, yellowish-white light profile, suggesting an older stellar population with minimal dust obscuration. This dominates the overall luminosity.

The other component appears more elongated, with a bluish-white hue. It seems to be a disk-like structure. The lack of well-defined spiral arms suggests either a smooth disk morphology or a disk galaxy viewed at a relatively high inclination angle. There is no apparent bulge within this disk.

Based on the faintness of the disk it seems to be undergoing only a low level of star formation.
