The galaxy exhibits an intermediate redshift. Morphologically, it displays characteristics of both a smooth and a featured galaxy. There appears to be a central bulge with a relatively smooth light distribution, possibly indicating an older stellar population. However, there are also hints of a disk component. The disk appears relatively undisturbed, but shows minor disturbances as it has unevenness in its spiral structure. There is evidence of a recent or ongoing merger event. There appear to be irregular structures indicating tidal effects due to gravitational interactions. The estimated mass of the galaxy is considerable, suggesting it is a fairly massive system. The colors suggest ongoing star formation, though it might not be very high, with possible redder regions indicating older stellar populations and bluer regions indicating active star formation. Overall, the galaxy appears to be in a transition state, possibly evolving from a disk-dominated system towards a more elliptical morphology due to an interaction or merger.
