This galaxy exhibits a morphology that suggests it may be the result of an ongoing or recent interaction. The overall structure appears generally smooth, however, there is evidence of a tidal tail or bridge-like feature extending from the main body. It is not definitively a clear merging event, although there are potential disturbances suggesting a minor interaction. The galaxy has a relatively round appearance. The core is concentrated with a yellow hue, suggesting an older stellar population. Overall the galaxy is a moderate spiral or elliptical. Based on its apparent magnitude in DESI bands (g, r, z), the estimated distance and redshift implies a substantially luminous system. The mass estimates also support a galaxy of a significant mass. The galaxy's star formation rates suggest that it is not a strong star-forming galaxy. Specific star formation rate appears quite low.
