This galaxy presents as a relatively faint, elongated spiral with a moderate redshift. It exhibits a bright central bulge, suggestive of a considerable stellar mass concentration. The disk of the galaxy appears relatively smooth, with only hints of spiral arm structure visible. These arms are loosely wound and somewhat diffuse, showing regions of bluer light, likely indicating areas of recent or ongoing star formation. There is some evidence of minor asymmetry or distortion in the disk, with the suggestion of tidal features and minor irregularities. Overall, this appears to be a galaxy with an intermediate mass, exhibiting moderate star formation activity within its disk. There appears to be indications of interactions but not anything major.
