The galaxy presents as a spiral type, viewed at an oblique angle.  Spiral arms appear present but are not sharply defined, exhibiting a somewhat flocculent structure.  There is a distinct central bulge with a yellowish hue, suggesting an older stellar population concentrated in the galactic nucleus.  The outer disk regions show a bluer tint, indicative of ongoing star formation. The galaxy is moderately luminous, and the apparent size suggests it is a dwarf galaxy. No significant tidal features or distortions are visible, suggesting it is relatively undisturbed.  A faint bar structure seems to extend through the central bulge. The overall morphology leans towards a galaxy with a small bulge component. There are some signs of minor disturbances, such as tidal tails or asymmetries. The galaxy is at an intermediate redshift and is likely low mass.
