The galaxy presents a largely smooth and rounded morphology. The central bulge exhibits a yellowish hue, suggesting an older stellar population. There appears to be a subtle disk structure present, but it is poorly defined. The galaxy shows a slight elongation, but generally appears circular in shape. There may be a minor disturbance, and evidence of a slight merger event. The overall color profile is dominated by redder wavelengths, indicative of a galaxy with comparatively low levels of ongoing star formation.
