The galaxy appears to be a relatively luminous object at a moderate redshift. It exhibits a morphology that is somewhat ambiguous, appearing neither completely smooth nor clearly disk-like. There is a central concentration of light, appearing yellowish, which suggests an older stellar population in the galactic bulge. The overall shape is moderately round, with some indication of a deviation from perfect ellipticity. Evidence suggests a possible minor disturbance in the galactic structure, possibly indicative of a past or ongoing minor merger event. There is a faint outer halo, with a bluer component toward the edges. The stellar mass of this galaxy is large, and the star formation rate is present, even if on the lower end. Overall, it is difficult to classify precisely but the galaxy presents characteristics of an intermediate type between elliptical and spiral, potentially a lenticular galaxy experiencing some tidal interaction.
