The galaxy presents as a moderately luminous object at a redshift of approximately 0.069. It exhibits a discernible disk structure, though not sharply defined. The overall form is more elliptical than a pure spiral, with a smooth, diffuse appearance dominating. There is a slight elongation, suggesting a deviation from a perfectly circular shape.

Evidence suggests an ongoing interaction or merging event. Faint tidal features or minor disturbances can be inferred, as there seems to be an irregular distribution of light on the edge of the galaxy, but that also might be caused by noise in the image. The color indices suggest that it may have an older stellar population, with a faint blue tinge near the center. Overall, the galaxy appears to be undergoing little to no star formation. The luminosity suggests a galaxy of considerable mass.
