The galaxy presents an interacting system, appearing as a close pair of objects exhibiting merging behavior. The system has a generally ellipsoidal morphology.

The larger component displays a primarily smooth texture and a yellowish-orange color profile, suggesting an older stellar population. The smaller, more compact component exhibits a similar yellowish-orange hue. A faint bluish-green tint towards the outer edges of the system hints at the presence of younger, hotter stars possibly triggered by the ongoing interaction. Faint tidal tails or bridges of material are not readily apparent, though the merging classification suggests these may exist at lower light levels or obscured by dust. The overall impression is of a dynamically active system in the process of transformation.
