The galaxy appears to be a relatively luminous, early-type spiral galaxy with a redshift of z ≈ 0.17. It is viewed at an oblique angle. The central bulge region is very bright and yellowish, likely indicating an older stellar population. There is a presence of spiral arm structures that extend outwards from the bulge. These arms appear slightly flocculent and show bluer hues, suggesting ongoing star formation. The outer disk region is less defined, appearing smoother and less structured. The overall morphology leans toward a smooth, rather than highly disturbed, appearance. The galaxy shows a moderate ellipticity, appearing somewhat elongated, but not extremely so. There's no apparent evidence of a major ongoing merger or significant tidal disruption.
