The galaxy presents an elongated morphology, with a notable asymmetry in its structure. A bright, concentrated central region is evident, possibly indicating a significant bulge component. This region displays a yellowish hue, suggesting a population of older stars.

Extending from this central region, a fainter, bluish structure is observed. The bluer color implies a younger stellar population and possible ongoing star formation within this structure. The overall form suggests a disturbed morphology, potentially resulting from a gravitational interaction or merger event. There's a chance of this galaxy being a spiral, but seen almost edge-on.

There are faint features on the outskirts of the galaxy that may be indicative of tidal tails or other debris resulting from the interaction. The system has a reddish hue, but due to the distance of the object, it could be redshift effects.
