The galaxy presents as a merging system, exhibiting significant morphological disturbance. A primary, relatively smooth component dominates, with a centrally concentrated, bright core exhibiting a bluish-white hue, suggestive of a population of younger, hotter stars. This central region appears slightly elongated.

Attached to the primary component is a secondary object. This has a yellowish to reddish color, indicating an older stellar population, and appears less concentrated than the primary's core. A tidal tail is visible, further indicating ongoing gravitational interaction. The overall shape of the system is highly irregular, not conforming to typical elliptical or spiral structures.
