This galaxy exhibits a disk-like morphology, appearing to be viewed at a significant inclination relative to our line of sight. The central region displays a concentrated, bright bulge. There is evidence of star formation, with a noticeable presence of regions exhibiting bluer light on one end of the disk. Conversely, the opposite end shows some light on the redder end of the spectrum. The galaxy appears relatively undisturbed, without any significant signs of tidal interactions or ongoing mergers, though there is some indication of minor disturbances. The overall structure suggests a spiral or lenticular galaxy type.
