This galaxy exhibits a morphology consistent with an ongoing or recent merger event. Two distinct luminous components are discernible, likely representing the cores of the merging galaxies. The overall color appears yellowish-orange, potentially indicating an older stellar population with lower rates of ongoing star formation. The galaxy appears relatively compact, with an estimated half-light radius of approximately 9 kpc. There are some faint features that could be tidal tails, although the resolution of the image makes it hard to discern these conclusively. The luminosity suggests a relatively massive system. There is an apparent distortion of the central region, further supporting the presence of a gravitational interaction.
