The galaxy presents a complex morphology, appearing to be undergoing an interaction or merger. The central region exhibits a bright, diffuse glow, potentially indicating a substantial concentration of older stellar populations. This central brightness fades into a more extended disk-like structure that shows signs of significant disturbance. A notable asymmetry is present in the disk. Patches of reddish hue, possibly regions of dust obscuration or ongoing star formation, are observed. The overall shape deviates noticeably from a regular elliptical or spiral form, suggesting gravitational influence or disruption caused by a merger event. Faint tidal features may be present, however the image does not provide enough clarity to be certain. Overall, this galaxy's structure hints at an ongoing or recent dynamic event that has shaped its observed features.
