The galaxy presents a morphology that suggests an interacting system, possibly in the early stages of a merger. One component appears as an elongated, slightly disturbed disk, exhibiting a smoother texture with a color gradient transitioning from redder hues at one end to slightly bluer tones at the other. The other component is significantly more compact and amorphous, possessing a brighter, more uniform luminosity with a mixed color profile. The overall structure indicates gravitational interaction, which is causing the disturbance of its morphology. The relatively smooth appearance and colors suggests an older stellar population dominates. There is evidence of star formation, but it does not appear to be a dominant feature.
