The galaxy presents an intermediate redshift, suggestive of considerable distance. It exhibits a complex morphology, appearing neither purely elliptical nor a well-defined spiral. There's a dominant central bulge, moderately bright, and a surrounding disk with some discernible features, with a relatively low inclination angle to our line of sight. Indications suggest the galaxy is undergoing some form of interaction or disturbance, possibly a minor merger or tidal interaction. The colour distribution is somewhat uneven, with a slightly redder hue in the central bulge and bluer tints in portions of the disk, suggestive of ongoing star formation. Overall, the galaxy appears to be of substantial mass.
