The observed galaxy presents as a barred spiral type. Its structure is dominated by a relatively faint, diffuse disk component. Spiral arms are apparent and moderately well-defined, exhibiting a somewhat flocculent morphology. Star formation appears active within the arms, indicated by the presence of several bright, blue regions likely corresponding to young star clusters or HII regions. The central bulge is not prominent, suggesting it is either relatively small or obscured by dust. There is a faint bar structure that extends through the center. The overall colour profile suggests a lower-mass system with continuing star formation. There appears to be no significant tidal disturbance.