The galaxy presents as a distorted, elongated structure. The primary body exhibits a reddish-orange hue, with a central concentration that suggests a bulge component. Adjacent to this main body is a fainter, less defined region with a bluer coloration. This suggests a possible interaction or tidal disturbance, potentially indicating ongoing or recent merger activity. The overall morphology departs significantly from a regular spiral or elliptical form, further supporting the likelihood of gravitational interaction influencing its shape and star formation.
