The galaxy presents as a merging or interacting system, comprised of at least two distinct components. One component appears more condensed and spherical, exhibiting a bright, concentrated core with a smooth, albeit indistinct, outer halo. The other component is more diffuse and elongated, possibly indicative of tidal distortion or ongoing interaction. Both components present a relatively blue hue, suggestive of recent or ongoing star formation activity, and are connected by a faint bridge of material. The overall system lacks clear spiral arm structure.
