The galaxy appears to be a relatively bright, elongated system, exhibiting characteristics of an early-type spiral or lenticular galaxy. The central region is dominated by a concentrated, yellowish bulge, suggesting an older stellar population. Moving outward from the center, there is a subtle disk component visible. The disk shows hints of bluer regions, potentially indicative of younger stars or ongoing star formation, although at a low rate. The overall morphology suggests the galaxy is not currently undergoing any major merging events. However, there are subtle disturbances in the outer regions of the disk, which may indicate a minor interaction. The galaxy is moderately massive, and its stellar mass is consistent with that of a typical galaxy at its redshift.
