The galaxy presents as an intermediate-type spiral, observed at a considerable distance, with a redshift of approximately 0.11. The central bulge appears somewhat prominent and smooth, suggesting a high degree of stellar population homogeneity or advanced age. The overall shape of the galaxy appears largely undisturbed, though there is evidence of some minor disturbances. There is also evidence of some merging in the galaxy. A faint disk structure can be discerned, though not sharply defined. The colour profile seems relatively blue in the center. There is a presence of active star formation within the galaxy.
